Metallic abundances in the planet-harboring G-type star HD 38529

Publications of the Astronomical Society of Japan

Volumn 53, Issue 2, 2001, Pages 315-320

  Sadakane, Kozo ^a   Ohkubo, Michiko ^a   Sato, Shizuka ^b   Osada, Kyoichi ^b   Takada Hidai, Masahide ^b   Masuda, Seiji ^c   Izumiura, Hideyuki ^d   Koyano, Hisashi ^d   Maehara, Hideo ^d   Norimoto, Yuji ^d   Okada, Takafumi ^d   Shimizu, Yasuhiro ^d   Uraguchi, Fumihiro ^d   Watanabe, Etsuji ^d   Yanagisawa, Kenshi ^d   Yoshida, Michitoshi ^d  

^a OSAKA KYOIKU UNIVERSITY   (Japan)

^b TOKAI UNIVERSITY   (Japan)

^c KYOTO UNIVERSITY   (Japan)

^d NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

Planetary systems; Stars: abundances; Stars: individual (HD 38529)

Indexed keywords

IRON; STARS;

ATMOSPHERIC PARAMETERS; METALLICS; PLANETARY SYSTEM; STAR: INDIVIDUAL (HD 38529); STARS ABUNDANCES; STARS: BE; STARS: INDIVIDUAL: PROXIMA CENTAURI;

SPECTROSCOPIC ANALYSIS;

EID: 0035616345     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/53.2.315     Document Type: Article

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