MOST photometry and modeling of the rapidly oscillating (roAp) star γ Equulei

Astronomy and Astrophysics

Volumn 480, Issue 1, 2008, Pages 223-232

  Gruberbauer, M ^a   Saio, H ^b   Huber, D ^a   Kallinger, T ^a   Weiss, W ^a   Guenther, B ^c   Kuschnig, R ^d   Matthews, M ^d   Moffat, J ^e   Rucinski, S ^f   Sasselov, D ^g   Walker, H ^d  

^a UNIVERSITY OF VIENNA   (Austria)

^b TOHOKU UNIVERSITY   (Japan)

^c SAINT MARY S UNIVERSITY   (Canada)

^d UNIVERSITY OF BRITISH COLUMBIA   (Canada)

^e UNIVERSITÉ DE MONTRÉAL   (Canada)

^f UNIVERSITY OF TORONTO   (Canada)

^g HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Methods: data analysis; Stars: chemically peculiar; Stars: individual: Equ; Stars: magnetic fields; Stars: oscillations

Indexed keywords

DATA REDUCTION; GEOMETRY; INTERPOLATION; MAGNETIC FIELDS;

CHEMICALLY PECULIAR; FIELD STRENGTH; HIGH PRECISION PHOTOMETRY;

PHOTOMETRY;

EID: 39849084771     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078830     Document Type: Article

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