Zobrazeno 1 - 10
of 106
pro vyhledávání: '"Fuentes-Carrera, I."'
Autor:
Sanchez-Cruces, M., Sardaneta, M. M., Fuentes-Carrera, I., Rosado, M., Cardenas-Martinez, N., Lara-Lopez, M. A.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 513, Issue 2, pp.1755-1773, 2022
We present Fabry-Perot observations in the H$\alpha$ and [S II] lines to study the kinematics of the Magellanic-type dwarf irregular galaxy NGC 1569, these observations allowed us to computed the H$\alpha$ velocity field of this galaxy. Doing a detai
Externí odkaz:
http://arxiv.org/abs/2209.06766
Autor:
Fuentes-Carrera, I., Rosado, M., Amram, P., Laurikainen, E., Salo, H., Gomez-Lopez, J. A., Castaneda, H. O., Bernal, A., Balkowski, C.
Publikováno v:
A&A 621, A25 (2019)
Encounters between galaxies modify their morphology, kinematics, and star formation (SF) history. The relation between these changes and external perturbations is not straightforward. The great number of parameters involved requires both the study of
Externí odkaz:
http://arxiv.org/abs/1811.04158
We present direct images in the H$\alpha$ and [SII]$\lambda \lambda$6717,6731 $\text{\AA}$ lines of the Galactic Supernova Remnant G109.1-1.0 (CTB 109). We confirm that the filaments detected are the optical counterpart of the X-ray and radio superno
Externí odkaz:
http://arxiv.org/abs/1709.07986
Autor:
Rosado, M., Gabbasov, R. F., Repetto, P., Fuentes-Carrera, I., Amram, P., Martos, M., Hernandez, O.
Publikováno v:
2013 AJ, 145, 135
We present a kinematical study of the nearly edge-on galaxy ESO 379-G006 that shows the existence of extraplanar ionized gas. With Fabry-Perot spectroscopy at H-alpha, we study the kinematics of ESO 379-G006 using velocity maps and position-velocity
Externí odkaz:
http://arxiv.org/abs/1302.3520
In this work we present scanning Fabry-Perot H$\alpha$ observations of the isolated interacting galaxy pair NGC 5278/79 obtained with the PUMA Fabry-Perot interferometer. We derived velocity fields and rotation curves for both galaxies. For NGC 5278
Externí odkaz:
http://arxiv.org/abs/1002.2264
Autor:
Verley, S., Rosado, M., Repetto, P., Gabbasov, R., Verdes-Montenegro, L., Bergond, G., Fuentes-Carrera, I., Durbala, A.
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 the velocity field and rotation curve of the galaxy
Externí odkaz:
http://arxiv.org/abs/0910.1187
Autor:
Rodrigues, M., Hammer, F., Flores, H., Puech, M., Liang, Y. C., Fuentes-Carrera, I., Nesvadba, N., Lehnert, M., Yang, Y., Amram, P., Balkowski, C., Cesarsky, C., Dannerbauer, H., Delgado, R., Guiderdoni, B., Kembhavi, A., Neichel, B., Östlin, G., Pozzetti, L., Ravikumar, C. D., Rawat, A., Alighieri, S. di Serego, Vergani, D., Vernet, J., Wozniak, H.
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 last 6 to 8 Gyr ago, and likely have formed a sign
Externí odkaz:
http://arxiv.org/abs/0810.0272
Publikováno v:
Astron.Astrophys.484:299-302,2008
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 rotation curves of simulated equal-mass galaxies sufferin
Externí odkaz:
http://arxiv.org/abs/0804.0533
Autor:
Puech, M., Flores, H., Hammer, F., Yang, Y., Neichel, B., Lehnert, M., Chemin, L., Nesvadba, N., Epinat, B., Amram, P., Balkowski, C., Cesarsky, C., Dannerbauer, H., Alighieri, S. di Serego, Fuentes-Carrera, I., Guiderdoni, B., Kembhavi, A., Liang, Y. C., Oestlin, G., Pozzetti, L., Ravikumar, C. D., Rawat, A., Vergani, D., Vernet, J., Wozniak, H.
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 that the scatter in the z~0.6 TFR is caused by gala
Externí odkaz:
http://arxiv.org/abs/0803.3002
Autor:
Neichel, B., Hammer, F., Puech, M., Flores, H., Lehnert, M., Rawat, A., Yang, Y., Delgado, R., Amram, P., Balkowski, C., Cesarsky, C., Dannerbauer, H., Fuentes-Carrera, I., Guiderdoni, B., Kembhavi, A., Liang, Y. C., Nesvadba, N., Ostlin, G., Pozzetti, L., Ravikumar, C. D., Alighieri, S. di Serego, Vergani, D., Vernet, J., Wozniak, H.
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 galaxies with Mstell from 1.5 to 15 10^10Msun and posses
Externí odkaz:
http://arxiv.org/abs/0803.2370