High-redshift elliptical galaxies: Are they (all) really compact?

Monthly Notices of the Royal Astronomical Society

Volumn 401, Issue 2, 2010, Pages 933-940

  Mancini, C ^a   Daddi, E ^b   Renzini, A ^a   Salmi, F ^b   McCracken, H J ^c   Cimatti, A ^d   Onodera, M ^b   Salvato, M ^e   Koekemoer, A M ^f   Aussel, H ^b   Floc'H, E Le ^b,g   Willott, C ^h   Capak, P ^e,i  

^a INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^b CEA SACLAY   (France)

^c INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^d UNIVERSITY OF BOLOGNA   (Italy)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f STScI   (United States)

^g UNIVERSITY OF HAWAII   (United States)

^h NATIONAL RESEARCH COUNCIL CANADA   (Canada)

ⁱ CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Galaxies: elliptical and lenticular, cD; Galaxies: evolution; Galaxies: formation; Galaxies: high redshift

Indexed keywords

COSMOLOGY; SIGNAL TO NOISE RATIO;

EARLY TYPES; ELLIPTICAL GALAXIES; ELLIPTICALS; GALAXIES: ELLIPTICAL AND LENTICULAR CD; GALAXIES:HIGH-REDSHIFT; GALAXY EVOLUTION; GALAXY FORMATIONS; HIGH-REDSHIFT; INDEX PROFILE; PROPERTY;

GALAXIES;

EID: 73649122004     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15728.x     Document Type: Article

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