Measuring stellar oscillations using equivalent widths of absorption lines

Monthly Notices of the Royal Astronomical Society

Volumn 280, Issue 4, 1996, Pages 1155-1161

  Bedding, T R ^a   Kjeldsen, H ^b   Reetz, J ^c   Barbuy, B ^d  

^a UNIVERSITY OF SYDNEY   (Australia)

^b AARHUS UNIVERSITY   (Denmark)

^c UNIVERSITY OF MUNICH   (Germany)

^d UNIVERSITY OF SÃO PAULO   (Brazil)

Author keywords

Stars: individual: Cen A (HR 5459); Stars: individual: Boo (HR 5235); Stars: oscillations; Sun: atmosphere; Sun: oscillations; Scuti

Indexed keywords

IRON COMPOUNDS; STARS;

BALMER LINES; STAR OSCILLATIONS; STAR: INDIVIDUAL: Α CEN A (HR 5459); STAR: INDIVIDUAL: Η BOO (HR 5235); STARS: INDIVIDUAL: PROXIMA CENTAURI; SUN: ATMOSPHERE; SUN: OSCILLATIONS; Α CEN A; Δ SCUTI;

TEMPERATURE DISTRIBUTION;

EID: 0000612927     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/280.4.1155     Document Type: Article

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