Can sodium abundances of A-type stars be reliably determined from Na I 5890/5896 lines?

Publications of the Astronomical Society of Japan

Volumn 61, Issue 5, 2009, Pages 1165-1178

  Takeda, Yoichi ^a   Kang, Dong Il ^b   Han, Inwoo ^c   Lee, Byeong Cheol ^c,d   Kim, Kang Min ^c  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b Gyeongsangnamdo Institute of Science Education   (South Korea)

^c Korea Astronomy and Space Science Institute (KASI)   (South Korea)

^d Kyungpook National University   (South Korea)

Author keywords

Stars: abundances; Stars: atmospheres; Stars: chemically peculiar; Stars: early type; Stars: rotation

Indexed keywords

SODIUM COMPOUNDS; VELOCITY;

ABUNDANCE ANALYSIS; D LINES; MAIN SEQUENCE STARS; NON-LTE; STARS ABUNDANCES; STARS: ATMOSPHERE; STARS: BE; STARS: CHEMICALLY PECULIAR; STARS: ROTATION; STARS:EARLY TYPE;

STARS;

EID: 72149102445     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/61.5.1165     Document Type: Article

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