The Kormendy relation of massive elliptical galaxies at z ∼ 1.5: Evidence for size evolution

Monthly Notices of the Royal Astronomical Society

Volumn 374, Issue 2, 2007, Pages 614-626

  Longhetti, M ^a   Saracco, P ^a   Severgnini, P ^a   Della Ceca, R ^a   Mannucci, F ^b   Bender, R ^c,d   Drory, N ^d,e   Feulner, G ^c,d,f   Hopp, U ^c,d  

^a INAF IASF MILANO   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^c UNIVERSITY OF MUNICH   (Germany)

^d MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^e UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^f POTSDAM INSTITUTE FOR CLIMATE IMPACT RESEARCH   (Germany)

Author keywords

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

Indexed keywords

LUMINANCE; MORPHOLOGY;

CLASSIFIEDS; DISC LIKES; EARLY TYPES; EFFECTIVE RADIUS; ELLIPTICAL GALAXIES; GALAXIES: ELLIPTICAL AND LENTICULAR CD; GALAXY EVOLUTION; GALAXY FORMATIONS; MORPHOLOGICAL ANALYSIS; SURFACE BRIGHTNESS;

GALAXIES;

EID: 33846138637     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.11171.x     Document Type: Article

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