On the co-existence of chemically peculiar Bp stars, slowly pulsating B stars and constant B stars in the same part of the HR diagram

Astronomy and Astrophysics

Volumn 466, Issue 1, 2007, Pages 269-276

  Briquet, M ^a,f   Hubrig, S ^b   De Cat, P ^c   Aerts, C ^a,d   North, P ^e   Scholler M ^b  

^a KU LEUVEN   (Belgium)

^b EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^c ROYAL OBSERVATORY OF BELGIUM   (Belgium)

^d RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

^e EPFL   (Switzerland)

^f FUND FOR SCIENTIFIC RESEARCH   (Belgium)

Author keywords

Stars: chemically peculiar; Stars: early type; Stars: fundamental parameters; Stars: individual: HD 175362; Stars: magnetic fields; Stars: oscillations

Indexed keywords

STARS: CHEMICALLY PECULIAR; STARS: EARLY-TYPE; STARS: FUNDAMENTAL PARAMETERS; STARS: INDIVIDUAL: HD 175362; STARS: MAGNETIC FIELDS;

MAGNETIC FIELD EFFECTS; NONLINEAR SYSTEMS; PARAMETER ESTIMATION; PHOTOMETRY;

STARS;

EID: 34347356426     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066940     Document Type: Article

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