Model atmospheres of magnetic chemically peculiar stars: A remarkable strong-field Bp SiCrFe star HD137509

Astronomy and Astrophysics

Volumn 487, Issue 2, 2008, Pages 689-696

  Shulyak, D ^a   Kochukhov, O ^b   Khan, S ^c,d  

^a UNIVERSITY OF VIENNA   (Austria)

^b UPPSALA UNIVERSITY   (Sweden)

^c UNIVERSITY OF WESTERN ONTARIO   (Canada)

^d SAINT MARY S UNIVERSITY   (Canada)

Author keywords

Stars: atmospheres; Stars: chemically peculiar; Stars: individual: HD 137509; Stars: magnetic fields

Indexed keywords

ASTROPHYSICS; CODES (STANDARDS); CODES (SYMBOLS); COMPUTATIONAL METHODS; EARTH ATMOSPHERE; GEOPHYSICS; LEAD; MAGNETIC FIELD EFFECTS; MAGNETIC FIELD MEASUREMENT; MAGNETIC FIELDS; MAGNETIC MATERIALS; MODAL ANALYSIS; PHOTOMETRY; RADIATION; RADIATIVE TRANSFER; STARS;

ABUNDANCE ANALYSIS; CHEMICALLY PECULIAR STARS; DEVELOPED MODEL; FUNDAMENTAL PARAMETERS; HIGH-RESOLUTION SPECTRUM; LINE-BY-LINE; METALLICITIES; MODEL ATMOSPHERE; MODEL PREDICTIONS; NON-MAGNETIC; PARAMETER DETERMINATION; REAL OBJECTS; SELF-CONSISTENCY; SOLAR ABUNDANCES; SPECTRAL LINES; SPECTROSCOPIC OBSERVATIONS; STARS: ATMOSPHERES; STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: HD 137509; STARS: MAGNETIC FIELDS; STELLAR MODEL ATMOSPHERES; STRONG FIELDS; STRONG MAGNETIC FIELDS; SURFACE MAGNETIC FIELDS; ZEEMAN SPLITTING;

ATMOSPHERIC SPECTRA;

EID: 48849110631     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20079134     Document Type: Article

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