Evolution of the anti-truncated stellar profiles of S0 galaxies since z = 0.6 in the SHARDS survey. I. Sample and methods

Bibcode
2017A&A...604A.119B
DOI
10.1051/0004-6361/201630282
Borlaff, A.; Eliche-Moral, M. Carmen; Beckman, John E.; Ciambur, Bogdan C.; Pérez-González, Pablo G.; Barro, Guillermo; Cava, Antonio; Cardiel, Nicolas
Referencia bibliográfica

Astronomy and Astrophysics, Volume 604, id.A119, 71 pp.

Fecha de publicación:
8
2017
Revista
Astronomy and Astrophysics
Número de autores
8
Número de autores del IAC
3
Número de citas
10
Número de citas referidas
10
Descripción
Context. The controversy about the origin of the structure of early-type S0-E/S0 galaxies may be due to the difficulty of comparing surface brightness profiles with different depths, photometric corrections and point spread function (PSF) effects (which are almost always ignored). Aims: We aim to quantify the properties of Type-III (anti-truncated) discs in a sample of S0 galaxies at 0.2
Proyectos relacionados
Poster Almeria Astronomy week
Estudios Cinemáticos, Estructurales y de Composición, de los Medios Interestelares e Intergalácticos
El objetivo básico del proyecto es investigar la evolución de las galaxias mediante el entendimiento de la interacción del medio interestelar y las estrellas. La técnica principal que utilizamos es la cinemática bidimensional de galaxias enteras observada por nuestro instrumento GHaFaS, un interferometro Fabry Perot en el telescopio William
Prof.
John E. Beckman
En ejecución
Tipo
Con árbitro
Formación y Evolución de Galaxias (FYEG)
Métodos
Galaxias

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