Analysis of the photospheric lines of the magnetic CP star HR 7575

Publications of the Astronomical Society of Japan

Volumn 51, Issue 1, 1999, Pages 23-37

  Kato, Ken Ichi ^a   Sadakane, Kozo ^b  

^a National Museum of Nature and Science   (Japan)

^b OSAKA KYOIKU UNIVERSITY   (Japan)

Author keywords

Abundances; Stars:Individual (HR 7575); Stars:Magnetic; Stars:Peculiar A

Indexed keywords

CHROMIUM COMPOUNDS; IRON COMPOUNDS; MAGNETISM; RARE EARTHS; TEMPERATURE;

ABUNDANCE; ASTROPHYSICAL OBSERVATORY; EFFECTIVE TEMPERATURE; HIGH DISPERSION; MODEL ATMOSPHERE; SPECTROGRAMS; STAR:INDIVIDUAL (HR 7575); STAR:PECULIAR A; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:PECULIAR; STAR: INDIVIDUAL (HR 7575); STAR: PECULIAR A;

STARS;

EID: 0033244793     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/51.1.23     Document Type: Article

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