The EROs at z < 1.5 in the Groth-Westphal field of the GOYA survey

Bibcode
2005RMxAC..24..270P
Prieto, M.; Balcells, M.; Domínguez-Palmero, L.; Cristóbal-Hornillos, D.; Erwin, P.; Eliche-Moral, C.; Abreu, D.
Referencia bibliográfica

II International GTC Workshop: Science with GTC 1st-light Instruments and the LMT (Eds. A. M. Hidalgo-Gámez, J. J. González, J. M. Rodríguez Espinosa, and S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 24, pp. 270-270 (2005) (http://www.astroscu.unam.mx/~rmaa/)

Fecha de publicación:
12
2005
Número de autores
7
Número de autores del IAC
0
Número de citas
1
Número de citas referidas
1
Descripción
The study of the Extremly Red Objects (EROs), is the importance for setting constraints on the first epoch of massive galaxy formation, for exploring the population of dust reddened starburst and for testing models of galaxy formation in general. They are defined as objects with I-K>4(Vega). The traditional picture identifies the EROs either with passively evolving elliptical galaxies, or with young starburst reddened dust.
Tipo
Sin árbitro
Galaxias
Formación estelar

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