Non-LTE abundance analyses of nitrogen and sulfur in chemically peculiar stars of the upper main sequence

Publications of the Astronomical Society of Japan

Volumn 48, Issue 5, 1996, Pages 739-752

  Takada Hidai, Masahide ^a,b   Takeda, Yoichi ^c  

^a TOKAI UNIVERSITY   (Japan)

^b NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^c UNIVERSITY OF TOKYO   (Japan)

Author keywords

Spectroscopy; Stars: Abundances; Stars: Atmospheres; Stars: Chemically peculiar stars; Stars: Early type

Indexed keywords

BINARY ALLOYS; INFRARED DEVICES; MANGANESE ALLOYS; MERCURY AMALGAMS; NITROGEN; SULFUR;

ABUNDANCE ANALYSIS; CHEMICALLY PECULIAR-STARS; CORRECTION FACTORS; NEAR-INFRARED SPECTRAL REGIONS; NON-LTE; STAR: CHEMICALLY PECULIAR STAR; STARS ABUNDANCES; STARS: ATMOSPHERE; STARS: CHEMICALLY PECULIAR; STARS:EARLY TYPE;

STARS;

EID: 0030300548     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/48.5.739     Document Type: Article

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