The distance to NGC 5904 (M 5) via the subdwarf main sequence fitting method

Astronomy and Astrophysics

Volumn 421, Issue 2, 2004, Pages 603-612

  Testa, V ^a   Chieffi, A ^b   Limongi, M ^a   Andreuzzi, G ^a,c   Marconi, G ^a,d  

^a INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^b CNR   (Italy)

^c TNG   (Spain)

^d EUROPEAN SOUTHERN OBSERVATORY   (Chile)

Author keywords

Galaxy: globular clusters: individual: NGC 5904 (M 5); Stars: distances

Indexed keywords

CALIBRATION; COLOR; COSMIC RAYS; DATA ACQUISITION; ERROR CORRECTION; INSTRUMENT COMPONENTS; PHASE SEQUENCE INDICATORS; PHOTOMETRY; TELESCOPES; WAVE FILTERS;

GLOBULAR CLUSTERS; NGC 5904; SEQUENCE FITTING METHOD; SUBDWARF STARS;

GALAXIES;

EID: 3042801371     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034498     Document Type: Article

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