Dynamics of the isolated galaxy CIG 0314 (2009)
Verley, S., Rosado, M., Repetto, P., Gabbasov, R., Verdes-Montenegro, L., Bergond, G., ...
In the context of the AMIGA project, we used Fabry-Perot observations in order to study the dynamics of the ionised gas in the isolated galaxy CIG 0314. From the Halpha observations, we could obtain...
Rodrigues, M., Hammer, F., Flores, H., Puech, M., Liang, Y. C., Fuentes-Carrera, I., ...
Intermediate mass galaxies (logM(Msun)>10) at z~0.6 are the likeliest progenitors of the present-day numerous population of spirals. There is growing evidence that they have evolved rapidly since the...
Evidence for metallicity spreads in three massive M 31 globular clusters (2008)
Fuentes-Carrera, I., Jablonka, P., Sarajedini, A., Bridges, T., Djorgovski, G., Meylan, G.
Aims. We quantify the intrinsic width of the red giant branches of three massive globular clusters in M 31 in a search for metallicity spreads within these objects. Methods. We present HST/ACS...
Rotation curve bifurcations as indicators of close recent galaxy encounters (2008)
Pedrosa, S., Tissera, P. B., Fuentes-Carrera, I., De Oliveira, C. Mendes
Rotation curves of interacting galaxies often show that velocities are either rising or falling in the direction of the companion galaxy. We seek to reproduce and analyse these features in the...
IMAGES-III: The evolution of the Near-Infrared Tully-Fisher relation over the last 6 Gyr (2008)
Puech, M., Flores, H., Hammer, F., Yang, Y., Neichel, B., Lehnert, M., ...
Using the multi-integral field spectrograph GIRAFFE at VLT, we have derived the K-band Tully-Fisher relation (TFR) at z~0.6 for a representative sample of 65 galaxies with emission lines. We confirm...
Neichel, B., Hammer, F., Puech, M., Flores, H., Lehnert, M., Rawat, A., ...
We present a first combined analysis of the morphological and dynamical properties for the Intermediate MAss Galaxy Evolution Sequence (IMAGES) sample. It is a representative sample of 52 z~0.6...
Images I. Strong evolution of galaxy kinematics since z=1 (2008)
Yang, Y., Flores, H., Hammer, F., Neichel, B., Puech, M., Nesvadba, N., ...
IMAGES. I. Strong evolution of galaxy kinematics since z = 1 (2008)
Yang, Y., Flores, H., Hammer, F., Neichel, B., Puech, M., Nesvadba, N., ...
Nearly half the stellar mass of present-day spiral galaxies has formed since z = 1, and galaxy kinematics is an ideal tool to identify the underlying mechanisms responsible for the galaxy mass...
Rodrigues, M., Hammer, F., Flores, H., Puech, M., Liang, Y. C., Fuentes-Carrera, I., ...
Context: Intermediate mass galaxies (> 1010 M_o) at z ~ 0.6 are the likeliest progenitors of the present-day, numerous population of spirals. There is growing evidence that they have evolved rapidly...
IMAGES. III. The evolution of the near-infrared Tully-Fisher relation over the last 6 Gyr (2008)
Puech, M., Flores, H., Hammer, F., Yang, Y., Neichel, B., Lehnert, M., ...
Using the multi-integral field spectrograph GIRAFFE at VLT, we have derived the K-band Tully-Fisher relation (TFR) at z ÃÅ 0.6 for a representative sample of 65 galaxies with emission lines...
Neichel, B., Hammer, F., Puech, M., Flores, H., Lehnert, M., Rawat, A., ...
We present a first combined analysis of the morphological and dynamical properties for the intermediate-mass Galaxy Evolution Sequence (IMAGES) sample. It is a representative sample of 52...
IMAGES I. Strong evolution of galaxy kinematics since z=1 (2007)
Yang, Y., Flores, H., Hammer, F., Neichel, B., Puech, M., Nesvadba, N., ...
(abbreviated) We present the first results of the ESO large program, ``IMAGES'' which aims at obtaining robust measurements of the kinematics of distant galaxies using the multi-IFU mode of GIRAFFE...
Seyfert's Sextet: A Slowly Dissolving Stephan's Quintet? (2007)
Durbala, A., Del Olmo, A., Yun, M. S., Rosado, M., Sulentic, J. W., Plana, H., ...
We present a multiwavelength study of the highly evolved compact galaxy group known as Seyfert's Sextet (HCG79: SS). We interpret SS as a 2-3 Gyr more evolved analog of Stephan's Quintet (HCG92: SQ)....
The isolated interacting galaxy pair NGC 5426/27 (Arp 271) (2006)
Fuentes-Carrera, I., Rosado, M., Amram, P., Dultzin-Hacyan, D., Cruz-Gonzalez, I., Salo, H., ...
We present H alpha observations of the isolated interacting galaxy pair NGC 5426/27 using the scanning Fabry-Perot interferometer PUMA. The velocity field, various kinematical parameters and rotation...
The isolated interacting galaxy pair NGC 5426/27 (Arp 271) (2003)
Fuentes-Carrera, I., Rosado, M., Amram, P., Dultzin-Hacyan, D., Cruz-Gonzalez, I., Salo, H., ...
We present H alpha observations of the isolated interacting galaxy pair NGC 5426/27 using the scanning Fabry-Perot interferometer PUMA. The velocity field, various kinematical parameters and rotation...
The isolated interacting galaxy pair NGC 5426/27 (Arp 271) (2003)
Fuentes-Carrera, I., Rosado, M., Amram, P., Dultzin-Hacyan, D., Cruz-Gonzalez, I., Salo, H., ...
We present H alpha observations of the isolated interacting galaxy pair NGC 5426/27 using the scanning Fabry-Perot interferometer PUMA. The velocity field, various kinematical parameters and rotation...
The isolated interacting galaxy pair NGC 5426/27 (Arp 271) (2003)
Fuentes-Carrera, I., Rosado, M., Amram, P., Dultzin-Hacyan, D., Cruz-Gonzalez, I., Salo, H., ...
We present H alpha observations of the isolated interacting galaxy pair NGC 5426/27 using the scanning Fabry-Perot interferometer PUMA. The velocity field, various kinematical parameters and rotation...