R. Napiwotzki

Details der Publikationsliste

Zeitraum

1993 - 2009

Anzahl

204

Co-Autoren

A survey for post common-envelope binary stars using GALEX and SDSS photometry (2009)

Maxted, P. F. L., Gaensicke, B. T., Burleigh, M. R., Southworth, J., Marsh, T. R., Napiwotzki, R., ...

We report the first results of our programme to obtain multi-epoch radial velocity measurements of stars with a strong far-UV excess to identify post common-envelope binaries (PCEBs). The targets...

High-resolution UVES/VLT spectra of white dwarfs observed for the ESO SN Ia Progenitor Survey. III. DA white dwarfs (2009)

Koester, D., Voss, B., Napiwotzki, R., Christlieb, N., Homeier, D., Lisker, T., ...

The ESO Supernova Ia Progenitor Survey (SPY) took high-resolution spectra of more than 1000 white dwarfs and pre-white dwarfs. About two thirds of the stars observed are hydrogen-dominated DA white...

The UV-Excess Survey of the Northern Galactic Plane (UVEX) (2009)

Groot, Paul J., Verbeek, K., Greimel, R., Irwin, M., Gonzalez-Solares, E., Gaensicke, B., ...

The UV-Excess Survey of the Northern Galactic Plane images a 10x185 degree wide band, centered on the Galactic Equator using the 2.5m Isaac Newton Telescope in four bands (U,g,r,HeI5875) down to...

A new detailed examination of white dwarfs in NGC3532 and NGC2287 (2009)

Dobbie, P. D., Napiwotzki, R., Burleigh, M. R., Williams, K., Sharp, R. G., Barstow, M. A., ...

We present the results of a photometric and spectroscopic study of the white dwarf candidate members of the intermediate age open clusters NGC3532 and NGC2287. Of the nine objects investigated, it is...

The astrophysics of ultra-compact binaries (2009)

Nelemans, G., Wood, M., Groot, P., Anderson, S., Belczynski, K., Benacquista, M., ...

This white paper briefly describes the astrophysics of ultra-compact binaries, with emphasis of the challenges and opportunities in the next decade.

High resolution optical spectroscopy of Praesepe white dwarfs (2009)

Casewell, S. L., Dobbie, P. D., Napiwotzki, R., Burleigh, M. R., Barstow, M. A., Jameson, R. F.

We present the results of a high resolution optical spectroscopic study of nine white dwarf candidate members of Praesepe undertaken with the VLT and UVES. We find, contrary to a number of previous...

Central Stars of Planetary Nebulae in IPHAS and SDSS (2009)

Weston, S., Napiwotzki, R., Sale, S.

Space densities and birthrates of Planetary Nebulae (PNe) are highly uncertain. A large range of formation rates has been derived by different studies, which has led to contradicting ideas for the...

The Age of White Dwarf Companions (2009)

Weston, S., Napiwotzki, R.

We carried out a spectroscopic investigation of single lined white dwarfs (WDs) in double degenerate (DD) systems and discuss their binary evolution. Simulated spectra of the Halpha region are used...

High spatial resolution Galactic 3D extinction mapping with IPHAS. (2009)

Sale, S.E., Drew, J.E., Unruh, Y.C., Irwin, M.J., Knigge, C., Phillips, S., ...

‘The definitive version is available at www3.interscience.wiley.com '. Copyright Blackwell Publishing / Royal Astronomical Society. DOI: 10.1111/j.1365-2966.2008.14083.x

High resolution UVES/VLT spectra of white dwarfs observed for the ESO SN Ia Progenitor Survey III. DA white dwarfs. (2009)

Koester, D., Voss, B., Napiwotzki, R., Christlieb, N., Homeier, D., Lisker, T., ...

Original article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory (ESO) DOI: 10.1051/0004-6361/200912531

High Spatial Resolution Galactic 3D Extinction Mapping with IPHAS (2008)

Sale, S. E., Drew, J. E., Unruh, Y. C., Irwin, M. J., Knigge, C., Phillipps, S., ...

We present an algorithm ({\scshape mead}, for `Mapping Extinction Against Distance') which will determine intrinsic ($r' - i'$) colour, extinction, and distance for early-A to K4 stars extracted from...

A planetary nebula around nova V458 Vul undergoing flash ionization (2008)

Wesson, R., Barlow, M. J., Corradi, R. L. M., Drew, J. E., Groot, P. J., Knigge, C., ...

Nova V458 Vul erupted on 2007 August 8th and reached a visual magnitude of 8.1 a few days later. H$\alpha$ images obtained six weeks before the outburst as part of the IPHAS galactic plane survey...

Discovery of a widely separated UCD-WD binary (2008)

Day-Jones, A. C., Pinfield, D. J., Napiwotzki, R., Burningham, B., Jenkins, J. S., Jones, H. R. A., ...

We present the discovery of the widest known ultracool dwarf - white dwarf binary. This binary is the first spectroscopically confirmed widely separated system from our target sample. We have used...

Model Spectra of Hot Subdwarfs for the Gaia Mission (2008)

Hindson, L., Napiwotzki, R., Heber, U., Lemke, M.

The Gaia mission will provide an unprecedented 3D view of our galaxy, it will obtain astrometric, photometric and spectrographic data for roughly one billion stars. We are particularly interested in...

Radial Velocity Variable sdO/Bs from SPY - Preliminary Orbits of Three New Short Period Binaries (2008)

Geier, S., Heber, U., Napiwotzki, R.

We present new results from follow-up time-resolved spectroscopy of radial velocity variable hot subdwarfs from the SPY project. Medium resolution spectra were taken at the ESO NTT. Preliminary...

Binary sdB Stars with Massive Compact Companions (2008)

Geier, S., Karl, C., Edelmann, H., Heber, U., Napiwotzki, R.

The masses of compact objects like white dwarfs, neutron stars and black holes are fundamental to astrophysics, but very difficult to measure. We present the results of an analysis of subluminous B...

Metal Abundances of Subdwarf B Stars from SPY - a Pattern Emerges (2008)

Geier, S., Heber, U., Napiwotzki, R.

The formation of sdBs is still puzzling, as is the chemical composition of their atmospheres. While helium and other light elements are depleted relative to solar values, heavy elements are highly...

LMC origin of the hyper-velocity star HE 0437-5439. Beyond the supermassive black hole paradigm (2008)

Przybilla, N., Nieva, M. F., Heber, U., Firnstein, M., Butler, K., Napiwotzki, R., ...

Context: Hyper-velocity stars move so fast that only a supermassive black hole (SMBH) seems to be capable to accelerate them. Hence the Galactic centre (GC) is their only suggested place of origin....

Recycling Matter in the Universe. X-ray observations of SBS 1150+599A (PN G135.9+55.9). (2008)

Tovmassian, G.H., Tomsick, J., Napiwotzki, R., Yungelson, L., Pena, M., Stasińska, G, ...

Original paper can be found at: http://proceedings.aip.org/proceedings/ Copyright AIP DOI: 10.1063/1.2840455

The Origin of Helium-Rich Subdwarf O Stars. (2008)

Napiwotzki, R.

Original paper can be found at: http://www.astrosociety.org/pubs/cs/381.html Copyright ASP

LMC origin of the hyper-velocity star HE 0437-5439: Beyond the supermassive black hole paradigm. (2008)

Przybilla, N., Nieva, M.A., Heber, U., Firnstein, M., Butler, K., Napiwotzki, R., ...

Original article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory DOI: 10.1051/0004-6361:200809391

Radial Velocity Variable sdO/Bs from SPY - Preliminary Orbits of Three New Short Period Binaries. (2008)

Geier, S., Heber, U., Napiwotzki, R.

Original paper can be found at: http://astrosociety.org/pubs/cs/381.html Copyright ASP

Binary sdB Stars with Massive Compact Companions. (2008)

Geier, S., Karl, C., Edelmann, H., Heber, U., Napiwotzki, R.

Original paper can be found at: http://astrosociety.org/pubs/cs/381.html Copyright ASP

Metal Abundances of Subdwarf B Stars from SPY - a Pattern Emerges. (2008)

Geier, S., Heber, U., Napiwotzki, R.

Original paper can be found at: http://astrosociety.org/pubs/cs/381.html Copyright ASP

Model Spectra of Hot Subdwarfs for the Gaia Mission. (2008)

Hindson, L., Napiwotzki, R., Heber, U., Lemke, M.

Original paper can be found at: http://astrosociety.org/pubs/cs/381.html Copyright ASP

Hypervelocity Stars: Young and Heavy or Old and Light? (2008)

Heber, U., Hirsch, H., Edelmann, H., Napiwotzki, R., O'Toole, S., Brown, W., ...

Original paper can be found at: http://astrosociety.org/pubs/cs/381.html Copyright ASP

Discovery of a widely separated ultracool dwarf–white dwarf binary. (2008)

Day-Jones, A.C., Pinfield, D.J., Napiwotzki, R., Burningham, B., Jenkins, J.S., Jones, H.R.A., ...

‘The definitive version is available at www.blackwell-synergy.com.’ Copyright Blackwell Publishing DOI: 10.1111/j.1365-2966.2008.13455.x

A planetary nebula around Nova V458 Vulpeculae undergoing flash ionization. (2008)

Wesson, R., Barlow, M.J., Corradi, R.L.M., Drew, J.E., Groot, P., Knigge, C., ...

Original article can be found at: http://www.iop.org/EJ/journal/apjl Copyright American Astronomical Society [Full text of this article is not available in the UHRA]

An object that defies stereotypes. X-ray observations of SBS 1150+599A -- the binary nucleus of PN G135.9+55.9 (2007)

Tovmassian, G., Tomsick, J., Napiwotzki, R., Yungelson, L., Stasińska, G., Peña, M., ...

We present X-ray observations of the close binary nucleus of the planetary nebula PN G135.9+55.9 obtained with the XMM satellite. The nebula is the most oxygen-poor PN known to date and is located in...

High-Resolution Spectra Observed for SPY. II. DB and DBA Stars (2007)

Voss, B., Koester, D., Napiwotzki, R., Christlieb, N., Reimers, D.

We present a detailed spectroscopic analysis of the stars with helium-dominated spectra in the ESO Supernova Ia Progenitor Survey (SPY). Atmospheric parameters, masses, and abundances of trace...

Six New ZZ Ceti Stars from the SPY and the HQS Surveys (2007)

Voss, B., Koester, D., Østensen, R., Napiwotzki, R., Homeier, D., Reimers, D.

We report on the discovery of six new ZZ Ceti stars. They were selected as candidates based on preparatory photometric observations of objects from the Hamburg Quasar Survey (HQS), and based on the...

A Debris Disk around the Central Star of the Helix Nebula? (2007)

Su, Kate Y. L., Rieke, G. H., Huggins, P. J., Gruendl, R., Napiwotzki, R., ...

Excess emission from a point-like source coincident with the central star of the Helix Nebula is detected with Spitzer at 8, 24, and 70 um. At 24 um, the central source is superposed on an extended...

The mass and radius of the M-dwarf in the short period eclipsing binary RR Caeli (2007)

Maxted, P. F. L., O'Donoghue, D., Morales-Rueda, L., Napiwotzki, R.

We present new photometry and spectroscopy of the eclipsing white dwarf - M-dwarf binary star RR Cae. We use timings of the primary eclipse from white-light photo-electric photometry to derive a new...

A debris disk around the central star of the Helix Nebula? (2007)

Su, K.Y.L., Chu, Y-H., Rieke, G., Huggins, P.J., Gruendl, R., Napiwotzki, R., ...

Original article can be found at: http://www.iop.org/EJ/journal/apjl Copyright American Astronomical Society DOI: 10.1086/513018 [Full text of this article is not available in the UHRA]

3D-Kinematics of White Dwarfs from the SPY-Project (2006)

Richter, R., Heber, U., Napiwotzki, R.

We present a progress report on the kinematical analysis of the entire SPY (ESO SN Ia Progenitor surveY) sample of about one thousand white dwarfs and hot subdwarfs. In a previous study (Pauli et al....

The subdwarf B + white dwarf binary KPD 1930+2752 - a Supernova Type Ia progenitor candidate (2006)

Geier, S., Nesslinger, S., Heber, U., Przybilla, N., Napiwotzki, R.

The nature of the progenitors of type Ia supernovae is still under controversial debate. KPD 1930+2752 is one of the best SN Ia progenitor candidates known today. The object is a double degenerate...

Spectroscopic Analysis of subluminous B Stars in Binaries with compact Companions (2006)

Geier, S., Karl, C., Edelmann, H., Heber, U., Napiwotzki, R.

The masses of compact objects like white dwarfs, neutron stars and black holes are fundamental to astrophysics, but very difficult to measure. We present the results of an analysis of subluminous B...

The fraction of DA white dwarfs with kilo-Gauss magnetic fields (2006)

Jordan, S., Cuadrado, R. Aznar, Napiwotzki, R., Schmid, H. M., Solanki, S. K.

Weak magnetic field has been searched for on only a small number of white dwarfs. Current estimates for white dwarfs with fields in excess of 1MG are about 10%; according to previous studies this...

The fraction of DA white dwarfs with kilo-Gauss magnetic fields (2006)

Jordan, S., Cuadrado, R. Aznar, Napiwotzki, R., Schmid, H. M., Solanki, S. K.

Current estimates for white dwarfs with fields in excess of 1MG are about 10%; according to our first high-precision circular-polarimetric study of 12 bright white dwarfs with the VLT (Aznar Cuadrado...

White dwarfs in the European Galactic Plane Surveys (EGAPS) (2006)

Morales-Rueda, L., Groot, P. J., Napiwotzki, R., Drew, J., Collaboration, The EGAPS

The space density of white dwarfs is highly uncertain even nearby. This results from the fact that the known sample of white dwarfs is largely incomplete in part because most white dwarfs have been...

Spectroscopic Analysis of Subluminous B Stars in Binaries - Four Candidate Systems with Neutron Star/Black Hole Companions Discovered (2006)

Geier, S., Karl, C., Edelmann, H., Heber, U., Napiwotzki, R.

The masses of compact objects like white dwarfs, neutron stars and black holes are fundamental to astrophysics, but very difficult to measure. We present the results of an analysis of subluminous B...

Recent observational progress in AM CVn binaries (2006)

Ramsay, G., Brocksopp, C., Groot, P., Hakala, P., Lehto, H., Marsh, T., ...

We present the results of some recent research on AM CVn systems. We present: X-ray/UV observations made using XMM-Newton; the X-ray grating spectrum of RX J1914+24; preliminary results of a search...

The hot subdwarf B + white dwarf binary KPD 1930+2752 - a Supernova Type Ia progenitor candidate (2006)

Geier, S., Nesslinger, S., Heber, U., Przybilla, N., Napiwotzki, R.

The nature of the progenitors of type Ia supernovae is still under controversial debate. KPD 1930+2752 is one of the best SN Ia progenitor candidates known today. The object is a double degenerate...

Hot subdwarfs from the ESO Supernova Ia Progenitor Survey: II. Atmospheric parameters of subdwarf O stars (2006)

Stroeer, A., Heber, U., Lisker, T., Napiwotzki, R., Dreizler, S., Christlieb, N., ...

We address the origin and evolutionary status of hot subdwarf stars by studying the optical spectral properties of 58 subdwarf O (sdO) stars. Combining them with the results of our previously studied...

A near-infrared spectroscopic detection of the brown dwarf in the post common envelope binary WD0137-349 (2006)

Burleigh, M. R., Hogan, E., Dobbie, P. D., Napiwotzki, R., Maxted, P. F. L.

We present a near-infrared spectrum of the close, detached white dwarf + brown dwarf binary WD0137-349 (Maxted et al 2006), that directly reveals the substellar companion through an excess of flux...

On the origin of the ultramassive white dwarf GD50 (2006)

Dobbie, P. D., Napiwotzki, R., Lodieu, N., Burleigh, M. R., Barstow, M. A., Jameson, R. F.

We argue on the basis of astrometric and spectroscopic data that the ultramassive white dwarf GD50 is associated with the star formation event that created the Pleiades and is possibly a former...

Survival of a brown dwarf after engulfment by a red giant star (2006)

Maxted, P. F. L., Napiwotzki, R., Dobbie, P. D., Burleigh, M. R.

(Summary of paper) High resolution optical spectroscopy of the white dwarf WD0137-349 reveals a weak Halpha line in emission, due to a low mass companion in a close orbit. Using this emission...

New Praesepe white dwarfs and the initial mass-final mass relation (2006)

Dobbie, P.D., Napiwotzki, R., Burleigh, Matthew R., Barstow, Martin A., Boyce, D.D., Casewell, S.L., ...

This is the preprint from arxiv.org of a paper subsequently published in the Monthly Notices of the Royal Astronomical Society and available from...

The peculiar sdB NGC6121-V46: A low-mass double degenerate ellipsoidal variable in a globular cluster (2006)

O'Toole, S. J., Napiwotzki, R., Heber, U., Drechsel, H., Frandsen, S., Grundahl, F., ...

The variable sdB known as V46 in the globular cluster M4 has remained enigmatic since its discovery almost 10 years ago. We present here radial velocity measurements obtained from medium-resolution...

New Praesepe white dwarfs and the initial mass-final mass relation (2006)

Dobbie, P. D., Napiwotzki, R., Burleigh, M. R., Barstow, M. A., Boyce, D. D., Casewell, S. L., ...

We report the spectroscopic confirmation of four further white dwarf members of Praesepe. This brings the total number of confirmed white dwarf members to eleven making this the second largest...

Spectroscopic Analysis of sdB Binaries from the SPY Project (2005)

Karl, C., Heber, U., Napiwotzki, R., Geier, S.

In the course of our search for double degenerate binaries as potential progenitors of type Ia supernovae with the ESO VLT (ESO SN Ia Progenitor SurveY SPY) several new subdwarf B (sdB) binaries with...

Time-resolved observations of the short period CV SDSS J123813.73-033933.0 (2005)

Zharikov, S. V., Tovmassian, G. H., Napiwotzki, R., Michel, R., Neustroev, V.

We observed a new and poorly studied cataclysmic variable (CV) SDSS J123813.73-033933.0 to determine its classification and binary parameters. Simultaneous time-resolved photometric and spectroscopic...

Discovery of eleven new ZZ Ceti stars (2005)

Castanheira, B. G., Kepler, S. O., Mullally, F., Winget, D. E., Koester, D., Voss, B., ...

We report the discovery of eleven new ZZ Cetis using telescopes at OPD (Observat\'orio do Pico dos Dias/LNA) in Brazil, the 4.1 m SOAR (Southern Astrophysical Research) telescope at Cerro Pachon,...

3D kinematics of white dwarfs from the SPY project II (2005)

Napiwotzki, R., Heber, U., Altmann, M., Odenkirchen, M.

We present the kinematics of a sample of 398 DA white dwarfs from the SPY project (ESO SN Ia Progenitor surveY) and discuss kinematic criteria for distinguishing thin-disk, thick-disk, and halo...

On the most metal-poor PN and its binary central star (2005)

Napiwotzki, R., Tovmassian, G., Richer, M. G., Stasinska, G., Pena, M., Drechsel, H., ...

PN G135.9+55.9 is the most metal-poor PN known in our Galaxy. The central star resides in a short-period binary system with a compact component, probably a white dwarf. We describe new observations,...

Rotation velocities of white dwarfs determined from the CaII K line (2005)

Berger, L., Koester, D., Napiwotzki, R., Reid, I. N., Zuckerman, B.

We determine projected rotation velocities v sini in DAZ white dwarfs, for the first time using the rotational broadening of the CaII K line. The results confirm previous findings that white dwarfs...

Wolf-Rayet and O Star Runaway Populations from Supernovae (2005)

Dray, L. M., Dale, J. E., Beer, M. E., Napiwotzki, R., King, A. R.

We present numerical simulations of the runaway fractions expected amongst O and Wolf-Rayet star populations resulting from stars ejected from binaries by the supernova of the companion....

Two new ZZ Ceti pulsators from the HS and HE surveys (2005)

Silvotti, R., Voss, B., Bruni, I., Koester, D., Reimers, D., Napiwotzki, R., ...

We report the detection of nonradial g-mode oscillations in the DA white dwarfs HS1039+4112 (B=15.9) and HE1429-0343 (B=15.8) from time-series photometry made at the Loiano 1.5 m telescope. The two...

Binaries discovered by the SPY project. IV. Five single-lined DA double white dwarfs (2005)

Nelemans, G., Napiwotzki, R., Karl, C., Marsh, T. R., Voss, B., Roelofs, G., ...

We present results from our ongoing follow-up observations of double white dwarf binaries detected in the ESO SN Ia Progenitor SurveY (SPY). We discuss our observing strategy and data analysis and...

Six detached white-dwarf close binaries (2005)

Morales-Rueda, L., Marsh, T. R., Maxted, P. F. L., Nelemans, G., Karl, C., Napiwotzki, R., ...

We determine the orbits of four double degenerate systems (DDs), composed of two white dwarfs, and of two white dwarf -- M dwarf binaries. The four DDs, WD1022+050, WD1428+373, WD1824+040, and...

Kilo-gauss Magnetic Fields in three DA White Dwarfs (2005)

Cuadrado, R. Aznar, Jordan, S., Napiwotzki, R., Schmid, H. M., Solanki, S. K., Mathys, G.

We have detected longitudinal magnetic fields between 2 and 4kG in three normal DA white dwarfs (WD0446-790, WD1105-048, WD2359$-$434) out of a sample of 12 by using optical spectropolarimetry done...

HE 0437-5439: an unbound hypervelocity main-sequence B-type star. (2005)

Edelmann, H., Napiwotzki, R., Heber, U., Christlieb, N., Reimers, D.

Original article can be found at: http://www.iop.org/EJ/journal/apjl Copyright American Astronomical Society DOI: 10.1086/498940 [Full text of this article is not available in the UHRA]

A near-IR spectroscopic search for very-low-mass cool companions to notable DA white dwarfs (2004)

Dobbie, P. D., Burleigh, M. R., Levan, A. J., Barstow, M. A., Napiwotzki, R., Holberg, J. B., ...

We have undertaken a detailed near-IR spectroscopic analysis of eight notable white dwarfs, predominantly of southern declination. In each case the spectrum failed to reveal compelling evidence for...

Identification of a DO White Dwarf and a PG1159 Star in the ESO SN Ia Progenitor Survey (SPY) (2004)

Werner, K., Rauch, T., Napiwotzki, R., Christlieb, N., Reimers, D., Karl, C. A.

We present high-resolution VLT spectra of a new DO white dwarf and a new PG1159 star, which we identified in the ESO SPY survey. The PG1159 star is a low-gravity, extremely hot (Teff=160,000 K, log...

Praesepe and the seven white dwarfs (2004)

Dobbie, P. D., Pinfield, D. J., Napiwotzki, R., Hambly, N. C., Burleigh, M. R., Barstow, M. A., ...

We report the discovery, from our preliminary survey of the Praesepe open cluster, of two new spectroscopically confirmed white dwarf candidate members. We derive the effective temperatures and...

3D-Kinematics of White Dwarfs from the SPY-Project (2004)

Pauli, E-M., Heber, U., Napiwotzki, R., Altmann, M., Odenkirchen, M.

We present kinematics of a sample of 398 DA white dwarfs from the SPY project (ESO SN Ia Progenitor surveY) and discuss kinematic criteria for a distinction of thin disk, thick disk, and halo...

Subluminous O stars from the ESO Supernova Progenitor Survey - Observation versus Theory (2004)

Stroeer, A., Heber, U., Lisker, T., Napiwotzki, R., Dreizler, S.

The ESO Supernova Progenitor Survey (SPY) has identified 58 (mostly helium-rich) subluminous O stars. We use the Balmer line strength to distinguish sdO from He-sdO (no Balmer lines) and present the...

Time-resolved observations of the short period CV SDSS J123813.73-033933 (2004)

Zharikov, S. V., Tovmassian, G. H., Neustroev, V., Michel, R., Napiwotzki, R.

We present simultaneous spectral and photometric observations of SDSS J123813.73-033933.0. From Ha radial velocity measurements we determined the orbital period of the system to be 0.05592+/-0.00002...

Hot subdwarfs from the ESO Supernova Ia Progenitor Survey - I. Atmospheric parameters and cool companions of sdB stars (2004)

Lisker, T., Heber, U., Napiwotzki, R., Christlieb, N., Han, Z., Homeier, D., ...

We present the analysis of a high-resolution, high-quality sample of optical spectra for 76 subdwarf B (sdB) stars from the ESO Supernova Ia Progenitor Survey (SPY). Effective temperature, surface...

A close binary nucleus in the most oxygen-poor planetary nebula PN G 135.9+55.9 (2004)

Tovmassian, G. H., Napiwotzki, R., Richer, M. G., Stasinska, G., Fullerton, A. W., Rauch, T.

We report FUSE and new deep optical spectroscopic observations of PN G 135.9+55.9, the most oxygen-poor planetary nebula located in the Galactic halo. These observations allow us to estimate the...

Identification of a DO white dwarf and a PG1159 star in the ESO SN Ia progenitor survey (SPY) (2004)

Werner, K., Rauch, T., Napiwotzki, R., Christlieb, N., Reimers, D., Karl, C. A.

We present high-resolution VLT spectra of a new helium-rich DO white dwarf and a new PG1159 star, which we identified in the ESO SPY survey. We performed NLTE model atmosphere analyses and found that...

Identification of neon in FUSE and VLT spectra of extremely hot hydrogen-deficient (pre-) white dwarfs (2004)

Werner, K., Rauch, T., Reiff, E., Kruk, J. W., Napiwotzki, R.

One of the strongest absorption lines observed in far-ultraviolet FUSE spectra of many PG1159 stars remained unidentified up to now. We show that this line, located at 973.3A, stems from NeVII. We...

Discovery of kilogauss magnetic fields in three DA white dwarfs (2004)

Cuadrado, R. Aznar, Jordan, S., Napiwotzki, R., Schmid, H. M., Solanki, S. K., Mathys, G.

We have detected longitudinal magnetic fields between 2 and 4 kG in three (WD 0446$-$790, WD 1105$-$048, WD 2359$-$434) out of a sample of 12 normal DA white dwarfs by using optical...

Double degenerates and progenitors of supernovae type Ia (2004)

Napiwotzki, R., Yungelson, L., Nelemans, G., Marsh, T. R., Leibundgut, B., Renzini, A., ...

We report on systematic radial velocity surveys for white dwarf - white dwarf binaries (double degenerates - DDs) including SPY (ESO Supernovae Ia progenitor survey) recently carried out at the VLT....

Spectral Types and Masses of White Dwarfs in Globular Clusters (2004)

Moehler, S., Koester, D., Zoccali, M., Ferraro, F. R., Heber, U., Napiwotzki, R., ...

White dwarfs in globular clusters offer additional possibilities to determine distances and ages of globular clusters, provided their spectral types and masses are known. We therefore started a...

Close binary EHB stars from SPY (2004)

Napiwotzki, R., Karl, C. A., Lisker, T., Heber, U., Christlieb, N., Reimers, D., ...

We present the results of a radial velocity (RV) survey of 46 subdwarf B (sdB) and 23 helium-rich subdwarf O (He-sdO) stars. We detected 18 (39%) new sdB binary systems, but only one (4%) He-sdO...

Close binary white dwarfs and supernovae IA (2004)

Christlieb , N., Drechsel , H., Heber , U., Homeier , D., Karl , C., Koester , D., ...

Informamos sobre el estado actual de los surveys" de velocidades radiales para binarias de enanas blancas (degeneradas dobles - DDs) incluyendo SPY (Exploración ESO de progenitoras de supernovas Ia)...

HS 2333 + 3927: a new sdB binary with a large reflection effect. (2004)

Karl, C., Heber, U., Drechsel, H., Napiwotzki, R., Altmann, M., Ostensen, R., ...

“The original publication is available at www.springerlink.com”. Copyright Springer. DOI: 10.1023/B:ASTR.0000044334.98860.ab [Full text of this article is not available in the UHRA]

FUSE Observations of EC14026 Stars. (2004)

Chayer, P., Fontaine, G., Fontaine, M., Lamontagne, R., Wesemael, F., Dupuis, J., ...

“The original publication is available at www.springerlink.com”. Copyright Springer. DOI: 10.1023/B:ASTR.0000044344.92680.b8 [Full text of this article is not available in the UHRA]

Spectroscopic analysis of sdB stars from the ESO Supernova Ia Progenitor Survey (2003)

Lisker, T., Heber, U., Napiwotzki, R., Christlieb, N., Reimers, D., Homeier, D.

We report on the analysis of high-resolution optical spectra for 77 subdwarf B (sdB) stars from the ESO Supernova Ia Progenitor Survey. Effective temperature, surface gravity, and photospheric helium...

Binaries discovered by the SPY project. III. HE2209-1444: a massive, short period double degenerate (2003)

Karl, C. A., Napiwotzki, R., Nelemans, G., Christlieb, N., Koester, D., Heber, U., ...

In the course of our search for double degenerate (DD) binaries as potential progenitors of type Ia supernovae with the UVES spectrograph at the ESO VLT (ESO SN Ia Progenitor surveY - SPY) we...

2MASSJ0516288+260738: Discovery of the first eclipsing late K + Brown dwarf system? (2003)

Schuh, S. L., Handler, G., Drechsel, H., Hauschildt, P. H., Dreizler, S., Medupe, R., ...

We report the discovery of a new eclipsing system less than one arcminute south of the pulsating DB white dwarf KUV 05134+2605. The object could be identified with the point source...

Spectral analysis of sdB stars from the Hamburg Quasar Survey (2003)

Edelmann, H., Heber, U., Lemke, M., Dreizler, S., Napiwotzki, R., ...

We present the results of a spectral analysis of a large sample of subdwarf B stars selected from follow-up observations of candidates from the Hamburg Quasar Survey. Fundamental parameters...

Heavy element abundance patterns in hot DA white dwarfs (2003)

Barstow, M. A., Good, S. A., Holberg, J. B., Hubeny, I., Bannister, N. P., Bruhweiler, F. C., ...

We present a series of systematic abundance measurements for 25 hot DA white dwarfs in the temperature range ~20000-110000K, based on far-UV spectroscopy with STIS/GHRS on HST, IUE and FUSE. Using...

3D kinematics of white dwarfs from the SPY project (2003)

Napiwotzki, R., Altmann, M., Heber, U., Odenkirchen, M., Kerber, F.

We present kinematics of a sample of 107 DA white dwarfs from the SPY project and discuss kinematic criteria for a distinction of thin disk, thick disk, and halo populations. This is the first...

Search for double degenerate progenitors of supernovae type Ia with SPY (2002)

Napiwotzki, R., Christlieb, N., Drechsel, H., Heber, U., Homeier, D., ...

We report on a large survey for double degenerate (DD) binaries as potential progenitors of type Ia supernovae with the UVES spectrograph at the ESO VLT (SN Ia Progenitor surveY - SPY). About 560...

Search for double degenerate progenitors of supernovae type Ia with SPY (2002)

Napiwotzki, R., Drechsel, H., Heber, U., Karl, C., Christlieb, N., ...

We report on a large survey for double degenerate (DD) binaries as potential progenitors of type Ia supernovae with the UVES spectrograph at the ESO VLT (ESO SN Ia Progenitor surveY - SPY).

Double degenerates from the supernova Ia progenitor survey (SPY) (2002)

Karl, C., Napiwotzki, R., Heber, U., Lisker, T., Nelemans, G., Christlieb, N., ...

We report on follow-up observations of double degenerate (DD) white dwarfs from the Supernovae Ia Progenitor Survey (SPY). Orbital parameters of four systems, including a massive short period system,...

Binaries discovered by the SPY project. II. HE 1414-0848: a double degenerate with a mass close to the Chandrasekhar limit (2002)

Napiwotzki, R., Koester, D., Nelemans, G., Yungelson, L., Christlieb, N., Renzini, A., ...

In the course of our search for double degenerate (DD) binaries as potential progenitors of type Ia supernovae with the UVES spectrograph at the ESO VLT (ESO SN Ia Progenitor surveY - SPY) we...

Search for progenitors of supnernovae type Ia with SPY (2002)

Napiwotzki, R., Christlieb, N., Drechsel, H., Heber, U., Homeier, D., ...

We have started a large survey for double degenerate (DD) binaries as potential progenitors of type Ia supernovae with the UVES spectrograph at the ESO VLT (ESO SN Ia Progenitor surveY - SPY). About...

Resolving subdwarf B stars in binaries by HST imaging (2002)

Heber, U., Moehler, S., Napiwotzki, R., Thejll, P., Green, E. M.

The origin of subluminous B stars is still an unsolved problem in stellar evolution. Single star as well as close binary evolution scenarios have been invoked but until now have met with little...

HS 0705+6700: a new eclipsing sdB binary (2001)

Drechsel, H., Heber, U., Napiwotzki, R., Ostensen, R., Johannessen, F., ...

We report the discovery of an eclipsing binary - HS 0705+6700 - being an sdB star with a faint companion. From its light curve the orbital period of 8263.87 s, the mass ratio of the system q = 0.28,...

Binaries discovered by the SPY project I. HE 1047-0436: a subdwarf B + white dwarf system (2001)

Napiwotzki, R., Edelmann, H., Heber, U., Karl, C., Drechsel, H., ...

In the course of our search for double degenerate binaries as potential progenitors of type Ia supernovae with the UVES spectrograph at the ESO VLT (ESO SN Ia Progenitor surveY - SPY) we discovered...

Metal abundances of sdB stars. (2001)

Edelmann, H., Heber, U., Napiwotzki, R.

Original article can be found at: http://www3.interscience.wiley.com Copyright WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim DOI: 10.1002/1521-3994(200112)322:5/63.0.CO;2-M Full text of this article is...

Search for progenitors of supernovae type Ia with SPY. (2001)

Napiwotzki, R., Christlieb, N., Drechsel, H., Hagen, H.J., Heber, U., Homeier, D., ...

‘The definitive version is available at www3.interscience.wiley.com .' Copyright WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim DOI: 10.1002/1521-3994(200112)322:5/63.0.CO;2-I [Full text of this...

Heavy element abundances in DA white dwarfs (2000)

Barstow, M. A., Burleigh, M. R., Bannister, N. P., Holberg, J. B., Hubeny, I., Bruhweiler, F. C., ...

We present a series of systematic abundance measurements for a group of hot DA white dwarfs in the temperature range 20,000-75,000K, based on far-UV spectroscopy with STIS on HST, IUE and FUSE. Using...

First VLT spectra of white dwarfs in a globular cluster (2000)

Moehler, S., Heber, U., Napiwotzki, R., Koester, D., Renzini, A.

We present the first spectra obtained with the Very Large Telescope for white dwarfs in a globular cluster. Estimates of atmospheric parameters are obtained and compared to evolutionary tracks. We...

Optical spectroscopy of the candidate luminous white dwarf in the young LMC cluster NGC1818 (1999)

Burleigh, M. R., Saffer, R. A., Gilmore, G. F., Napiwotzki, R.

An optical spectrum of the Elson et al. (1998) candidate luminous white dwarf in the young LMC cluster NGC1818 shows conclusively that it is not a degenerate star. A model atmosphere fit gives...

Abundances of UV bright stars in globular clusters. I. ROA 5701 in omega Centauri and Barnard 29 in M 13 (1998)

Moehler, S., Heber, U., Lemke, M., Napiwotzki, R.

Two UV brights stars in globular clusters, ROA 5701 (omega Cen) and Barnard 29 (M 13) are analysed from high-resolution UV and optical spectra. The main aim is the measurement of iron abundances from...

The UV bright star ZNG 1 in M 5 (1998)

Napiwotzki, R., Heber, U.

We report the results of H_alpha imaging and UV spectroscopy with the Hubble Space Telescope of the hot post-AGB star ZNG 1 in M 5 and its suspected planetary nebula.

Hot UV bright stars in globular clusters (1998)

Moehler, S., Landsman, W., Napiwotzki, R.

We have obtained medium-resolution spectra of seven UV-bright stars discovered on images of four southern globular clusters obtained with the Ultraviolet Imaging Telescope (UIT). Effective...

Temperature determination of the cool DO white dwarf HD149499B from EUVE observations (1996)

Jordan, S., Napiwotzki, R., Koester, D., Rauch, T.

We present a LTE model atmosphere analysis of the medium and long wavelength spectrum of the cool DO white dwarf HD149499B. This observation in the spectral range 230-700 A supplements a previous...