Star counts in the galaxy simulating from very deep to very shallow photometric surveys with the TRILEGAL code

Astronomy and Astrophysics

Volumn 436, Issue 3, 2005, Pages 895-915

  Girardi, L ^a   Groenewegen, M A T ^b   Hatziminaoglou, E ^c,d   Da Costa, L ^c  

^a INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^b KU LEUVEN   (Belgium)

^c EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^d INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

Author keywords

Galaxy: Stellar content; Galaxy: Structure; M diagrams; Russell (HR) C; Stars: Hertzsprung; Stars: Luminosity function, mass function; Surveys

Indexed keywords

ABSORPTION; APPROXIMATION THEORY; COLOR; COMPUTER SIMULATION; DATA REDUCTION; PHOTOMETRY;

HERTZSPRUNG-RUSSELL (HR) AND C-M DIAGRAMS - SURVEYS - GALAXY; LUMINOSITY FUNCTION, MASS FUNCTION - STARS; STARS; STELLAR CONTENT - GALAXY; STRUCTURES;

GALAXIES;

EID: 21244451109     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20042352     Document Type: Article

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