The influence of chemical composition on the properties of Cepheid stars I. Period-Luminosity relation vs. iron abundance

Astronomy and Astrophysics

Volumn 429, Issue 2, 2005, Pages

  Romaniello, M ^a   Primas, F ^a   Mottini, M ^a   Groenewegen, M ^b   Bono, G ^c   Francois P ^d  

^a EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^b KU LEUVEN   (Belgium)

^c INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^d UNIVERSITÉ PARIS DIDEROT   (France)

Author keywords

Cepheids; Stars: abundances; Stars: distances

Indexed keywords

CLOUDS; DATA REDUCTION; GALAXIES; IRON; MATHEMATICAL MODELS; PIPELINES; SPECTRUM ANALYSIS; STORMS;

CEPHEIDS; PERIOD-LUMINOSITY (PL) RELATION; STAR:ABUNDANCES; STAR:DISTANCES;

ASTROPHYSICS;

EID: 11144228441     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:200400110     Document Type: Article

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