Using cepheids to determine the galactic abundance gradient II. Towards the galactic center

Astronomy and Astrophysics

Volumn 384, Issue 1, 2002, Pages 140-144

  Andrievsky, S M ^a,b   Bersier, D ^c   Kovtyukh, V V ^b   Luck, R E ^d   Maciel, W J ^a   Lepine J R D ^a   Beletsky, Yu V ^b  

^a UNIVERSITY OF SÃO PAULO   (Brazil)

^b ODESSA NATIONAL UNIVERSITY   (Ukraine)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d CASE WESTERN RESERVE UNIVERSITY   (United States)

Author keywords

Galaxy: Abundances; Galaxy: Evolution; Stars: Abundances; Stars: Cepheids

Indexed keywords

GALAXIES; OBSERVATORIES; OPTICAL RESOLVING POWER; SIGNAL TO NOISE RATIO; SPACE TELESCOPES; SPECTROGRAPHS;

CEPHEIDS; GALACTIC DISC; STARS;

ASTROPHYSICS;

EID: 0036495360     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20020016     Document Type: Article

References (18)