Confirmation of the oblique pulsator model for the rapidly oscillating Ap star HR 3831

Monthly Notices of the Royal Astronomical Society

Volumn 300, Issue 4, 1998, Pages

  Baldry, I K ^a   Kurtz, D W ^b   Bedding, T R ^a  

^a UNIVERSITY OF SYDNEY   (Australia)

^b UNIVERSITY OF CAPE TOWN   (South Africa)

Author keywords

Stars: chemically peculiar; Stars: individual: HR 3831; Stars: oscillations; Stars: variables: other

Indexed keywords

STARS;

AMPLITUDE-MODULATED; PHOTOMETRIC VARIATIONS; RADIAL VELOCITY; STAR OSCILLATIONS; STAR: INDIVIDUAL: HR 3831; STAR: VARIABLE: OTHER; STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: VARIABLES; VELOCITY VARIATIONS;

PHOTOMETRY;

EID: 0006315354     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.00039.x     Document Type: Article

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