The determination of the rotational periods of the rapidly oscillating Ap stars from their mean light variations - V. An improved rotation period for the dipole pulsator HD 6532

Monthly Notices of the Royal Astronomical Society

Volumn 280, Issue 1, 1996, Pages 1-5

  Kurtz, D W ^a   Marang, F ^b   Van Wyk, F ^b   Roberts, G ^b  

^a UNIVERSITY OF CAPE TOWN   (South Africa)

^b SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

Author keywords

Stars: individual: HD 6532; Stars: oscillations; Stars: peculiar; Stars: rotation; Stars: variables: other

Indexed keywords

ROTATION;

FREQUENCY ANALYSIS; ROTATION FREQUENCIES; ROTATION PERIOD; STAR OSCILLATIONS; STAR: INDIVIDUAL: HD 6532; STAR: VARIABLE: OTHER; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: ROTATION; STARS: VARIABLES; STARS:PECULIAR;

STARS;

EID: 0041827740     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/280.1.1     Document Type: Article

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