GMASS ultradeep spectroscopy of galaxies at z ̃ 2 II. Superdense passive galaxies: How did they form and evolve?

Astronomy and Astrophysics

Volumn 482, Issue 1, 2008, Pages 21-42

  Cimatti, A ^a   Cassata, P ^b   Pozzetti, L ^c   Kurk, J ^d   Mignoli, M ^c   Renzini, A ^e   Daddi, E ^f   Bolzonella, M ^c   Brusa, M ^g   Rodighiero, G ^h   Dickinson, M ⁱ   Franceschini, A ^h   Zamorani, G ^c   Berta, S ^f   Rosati, P ^j   Halliday, C ^k  

^a UNIVERSITY OF BOLOGNA   (Italy)

^b OBSERVATOIRE DE MARSEILLE   (France)

^c OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^d MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^e INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^f CEA SACLAY   (France)

^g MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^h UNIVERSITY OF PADOVA   (Italy)

ⁱ NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^j EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^k INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

more..

Author keywords

Cosmology: observations; Galaxies: distances and redshifts; Galaxies: elliptical and lenticular, cD; Galaxies: evolution; Galaxies: formation; Galaxies: high redshift

Indexed keywords

GALAXIES; LUMINANCE; PHOTOMETRY; ULTRAVIOLET VISIBLE SPECTROSCOPY;

MASS DENSITIES;

COSMOLOGY;

EID: 42149164333     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078739     Document Type: Article

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