Zobrazeno 1 - 10
of 73
pro vyhledávání: '"Javier Gorgas"'
Autor:
Patricia Sanchez-Blazquez, A. Vazdekis, Jesús Falcón-Barroso, C. Allende Prieto, Anne E. Sansom, Javier Gorgas, A. de C. Milone, A. E. García Pérez, I. Martín Navarro, R. Cacho
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
instname
Extragalactic astronomy and stellar astrophysics are intrinsically related. In fact, the determination of important galaxy properties such as stellar masses, star formation histories, or chemical abundances relies on the ability to model their stella
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::03c407e7b929f6d0a369dc8cc0b1fdbf
https://eprints.ucm.es/id/eprint/67988/
https://eprints.ucm.es/id/eprint/67988/
Autor:
Alexandre Y. K. Bouquin, Javier Gorgas, Johan H. Knapen, Bililign T. Dullo, Armando Gil de Paz
Publikováno v:
The Astrophysical Journal
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
[Abridged] Tight correlations between supermassive black hole (SMBH) mass ($M_{\rm BH}$) and the properties of the host galaxy have useful implications for our understanding of the growth of SMBHs and evolution of galaxies. Here, we present newly obs
Autor:
Harald Kuntschner, Nicolás Cardiel, Scott Trager, Javier Gorgas, David R. Silva, A. Vazdekis, Reynier Peletier, E. Mármol-Queraltó, A. J. Cenarro, Patricia Sanchez-Blazquez
Publikováno v:
Astrophysical Journal Letters, 705(2), L199-L203. IOP PUBLISHING LTD
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
The study of stellar populations in early-type galaxies in different environments is a powerful tool for constraining their star formation histories. This study has been traditionally restricted to the optical range, where dwarfs around the turn-off
Autor:
Jesús Falcón-Barroso, Nicolás Cardiel, A. J. Cenarro, Michael A. Beasley, Reynier Peletier, Patricia Sanchez-Blazquez, Javier Gorgas, A. Vazdekis
Publikováno v:
Stellar Populations: Planning for the Next Decade, Proceedings of the International Astronomical Union, 262, 65-68
We present SEDs for single-age, single-metallicity stellar populations (SSPs) covering the full optical spectral range at resolution (FWHM = 2.3Å). These SEDs can be regarded as our base models, as we combine scaled-solar isochrones with an empirica
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Using the near-infrared spectral stellar library of Cenarro et al. (2001a,b), the behaviours of the Mg I line at 8807 angstrom and nearby TiO bands are analyzed in terms of the effective temperature, surface gravity, and metallicity of the library st
Autor:
Patricia Sanchez-Blazquez, Rafael Guzman, Nicolás Cardiel, Nicolas Gruel, Ana Matkovic, Javier Gorgas
Publikováno v:
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
We present line-strength measurements for 74 early-type galaxies in the core of the Coma cluster reaching down to velocity dispersions, sigma, of 30 km/s. The index-sigma relations for our sample, including galaxies with sigma
Accepted For Publi
Accepted For Publi
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
This is the first paper presenting our long-term project aimed at studying the nature of bulges through the analysis of their stellar population gradients. We present deep spectroscopic observations along the minor axis and the data reduction for a s
Autor:
Javier Gorgas, M. den Brok, E. Toloba, A. Rys, P. Guhathakurta, Sanjaya Paudel, Heikki Salo, Jesús Falcón-Barroso, Andrew J. Benson, J. Janz, T. Lisker, Reynier Peletier, S. Boissier, G. van de Ven, A. Boselli, Joshua J. Adams, Gerhard Hensler, Eija Laurikainen, E. Emsellem, J. D. Simon
Publikováno v:
The Astrophysical Journal, 799(2). IOP PUBLISHING LTD
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2015, 799 (2), ⟨10.1088/0004-637X/799/2/172⟩
The Astrophysical Journal, 2015, 799 (2), ⟨10.1088/0004-637X/799/2/172⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2015, 799 (2), ⟨10.1088/0004-637X/799/2/172⟩
The Astrophysical Journal, 2015, 799 (2), ⟨10.1088/0004-637X/799/2/172⟩
International audience; We analyze the stellar kinematics of 39 dwarf early-type galaxies (dEs) in the Virgo Cluster. Based on the specific stellar angular momentum lambda(Re) and the ellipticity, we find 11 slow rotators and 28 fast rotators. The fa
Publikováno v:
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
Aims: This paper commences a series devoted to the study of the stellar content of early-type galaxies. The goal of the series is to set constraints on the evolutionary status of these objects. Methods: In this paper we describe the details of the ga
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
We present line-strength gradients for 22 spectral indices measured in a sample of 82 early-type galaxies in different environments,including the high-density core of the Coma cluster, the Virgo cluster,poor groups,and field galaxies. We derive age a