Voss, R., Diehl, R., Hartmann, D. H., Cervino, M., Vink, J. S., Meynet, G., ...
We developed a new population synthesis code for groups of massive stars, where we model the emission of different forms of energy and matter from the stars of the association. In particular, the...
Sulphur in the Globular Clusters 47 Tucanae and NGC 6752 (2009)
Sbordone, L., Limongi, M., Chieffi, A., Caffau, E., Bonifacio, P.
The light elements Li, O, Na, Al, and Mg are known to show star to star variations in the globular clusters 47 Tuc and NGC 6752. Such variations are interpreted as due to processing in a previous...
Astrophysics with Radioactive Atomic Nuclei (2009)
Diehl, R., Von Ballmoos, P., Boggs, S., Burkert, A., Chieffi, A., Gehrels, N., ...
We propose to advance investigations of electromagnetic radiation originating in atomic nuclei beyond its current infancy to a true astronomy. This nuclear emission is independent from conditions of...
The peculiar type Ib supernova 2006jc: a WCO Wolf-Rayet star explosion (2008)
Tominaga, N., Limongi, M., Suzuki, T., Tanaka, M., Nomoto, K., Maeda, K., ...
The Peculiar Type Ib Supernova 2006jc: A WCO Wolf-Rayet Star Explosion (2007)
Tominaga, N., Limongi, M., Suzuki, T., Tanaka, M., Nomoto, K., Maeda, K., ...
We present a theoretical model for Type Ib supernova (SN) 2006jc. We calculate the evolution of the progenitor star, hydrodynamics and nucleosynthesis of the SN explosion, and the SN bolometric light...
RevMexAA (Serie de Conferencias), 10, 157--162 (2001) (2007)
Extreme Type Iip, P. Höflich, O. Straniero, M. Limongi, I. Dominguez, A. Chieffi
Evolutionary e#ects with redshift of core collapse supernovae and their application to cosmology have been studied based on an extensive grid of stellar models between 13 and 25 M# , and their light...
Extreme Type IIp Supernovae as Yardsticks for Cosmology (2006)
P. Höflich, O. Straniero, M. Limongi, I. Dominguez, A. Chieffi
Extreme Type IIp Supernovae as Yardsticks for Cosmology
Nucleosynthesis In Core Collapse Supernovae (2006)
We present the basic properties of the yields of our latest set of presupernova evolution and explosive nucleosynthesis of massive stars in the range between 11 and 120 Msun having solar and zero...
Nucleosynthesis of Fe60 in massive stars (2005)
We discuss at some extent the production of Fe60 in massive stars in the range between 11 and 120 Msun both in the hydrostatic and explosive stages. We also compare the Fe60/Al26 gamma-ray line flux...
On the origin of fluorine in the Milky Way (2004)
Renda, A., Fenner, Y., Gibson, B. K., Karakas, A. I., Lattanzio, J. C., Campbell, S., ...
The main astrophysical factories of fluorine (19F) are thought to be Type II supernovae, Wolf-Rayet stars, and the asymptotic giant branch (AGB) of intermediate mass stars. We present a model for the...
Evolution and nucleosynthesis of primordial low mass stars (2003)
Picardi, I., Chieffi, A., Limongi, M., Pisanti, O., Miele, G., Mangano, G., ...
We discuss in detail the evolutionary properties of low mass stars M< 1 M(Solar) having metallicity lower than Z=10^(-6) from the pre- main sequence up to (almost) the end of the Asymptotic Giant...
The Chemical Evolution of Magnesium Isotopic Abundances in the Solar Neighbourhood (2003)
Fenner, Y., Gibson, B. K., Karakas, A. I., Lattanzio, J. C., Chieffi, A., ...
The abundance of the neutron-rich magnesium isotopes observed in metal-poor stars is explained quantitatively with a chemical evolution model of the local Galaxy that considers - for the first time -...
Theoretical Light Curves of Type II-P SNe and Applications to Cosmology (2003)
Chieffi, A., Dominguez, I., Hoeflich, P., Limongi, M., Straniero, O.
Based on an extensive grid of stellar models between 13 and 25 Mo and a wide range of metallicities, we have studied the light curves of core collapse supernovae, their application to cosmology and...
Evolution, Explosion and Nucleosynthesis of Core Collapse Supernovae (2003)
We present a new set of presupernova evolutions and explosive yields of massive stars of initial solar composition (Y=0.285, Z=0.02) in the mass range 13-35 Msun. All the models have been computed...
The lithium content of the globular cluster NGC 6397 (2002)
Bonifacio, P., Pasquini, L., Spite, F., Bragaglia, A., Carretta, E., Castellani, V., ...
We make use of high resolution, high signal-to-noise ratio spectra of 12 turn-off stars in the metal-poor globular cluster NGC 6397 to measure its lithium content. We conclude that they all have the...
Abia, C., Dominguez, I., Straniero, O., Limongi, M., Chieffi, A., Isern, J.
Motivated by the recent detection of metals in different components of the high redshift universe and by the abundance ratios measured in the extremely metal-poor stars of our Galaxy, we study the...
Extreme type iip supernovae as yardsticks for cosmology (2001)
Chieffi , A., Dominguez , I., Höflich , P., Limongi , M., Straniero , O.
The O-Na and Mg-Al Anticorrelations in Turn-Off and early Subgiants in Globular Clusters (2000)
Gratton, R. G., Bonifacio, P., Bragaglia, A., Carretta, E., Castellani, V., Centurion, M., ...
High dispersion spectra (R>40,000) for a quite large number of stars at the main sequence turn-off and at the base of the subgiant branch in NGC6397 and NGC6752 were obtained with the UVES on Kueyen...
Extreme Type IIp Supernovae as Yardsticks for Cosmology (2000)
Höflich, P., Straniero, O., Limongi, M., Dominguez, I., Chieffi, A.
Evolutionary effects with redshift of core collapse supernovae and their application to cosmology have been studied based on an extensive grid of stellar models between 13 and 25 Mo, and their light...
Limongi, M., Straniero, O., Chieffi, A.
We present the evolutionary properties of a set of massive stellar models (namely 13, 15, 20 and 25 $\rm M_\odot$) from the main sequence phase up to the onset of the iron core collapse. All these...
Do zero metal intermediate mass stars experience thermal pulses? (1999)
Dominguez, I., Straniero, O., Limongi, M., Chieffi, A.
We have studied the evolution of intermediate mass (M.ge.5Mo) zero metal (Z=0) stars with particular attention to the AGB phase. At variance with previous claims we find that these stars experience...
Thermally Pulsing AGB Models of Intermediate Mass Stars (1999)
Straniero, O., Limongi, M., Chieffi, A., Dominguez, I., Busso, M., Gallino, R.
We present a set of models of AGB stars with initial mass larger than 5 Mo as obtained with the FRANEC code. It includes models of Z=0.02 and Z=0.001, with and without mass loss.
Ferraro, F. R., Messineo, M., Pecci, F. Fusi, De Palo, M. A., Straniero, O., Chieffi, A., ...
A catalog including a set of the most recent Color Magnitude Diagrams (CMDs) is presented for a sample of 61 Galactic Globular Clusters (GGCs). We used this data-base to perform an homogeneous...
The Luminosity Function of M3 (1999)
Rood, R. T., Carretta, E., Paltrinieri, B., Ferraro, F. R., Pecci, F. Fusi, Dorman, B., ...
We present a high precision, large sample luminosity function (LF) for the Galactic globular cluster M3. With a combination of ground based and Hubble Space Telescope data we cover the entire radial...
s-process nucleosynthesis in intermediate AGB stars. (1999)
Vaglio, P., Gallino, R., Busso, M., Travaglio, C., Straniero, O., Chieffi, A., ...
Prantzos, N. [Hrsg.]
Gallino, R., Arlandini, C., Busso, M., Lugaro, M., Travaglio, C., Straniero, O., ...
The Astrophysical Journal, 497(1998) S.388-403
Käppeler, F., Wiescher, M., Giesen, U., Görres, J., Baraffe, I., El Eid, M., ...
The Astrophysical Journal, 437(1994) S.396-409