The p-mode spectrum of γ Equ (HR 8097)

Monthly Notices of the Royal Astronomical Society

Volumn 282, Issue 1, 1996, Pages 243-251

  Martinez, Peter ^a   Weiss, W W ^b   Nelson, M J ^c   Kreidl, T J ^d   Roberts, G R ^e   Mkrtichian, D E ^f   Dorokhov, N I ^f   Dorokhova, T N ^f   Birch, P V ^g  

^a UNIVERSITY OF CAPE TOWN   (South Africa)

^b Institut fur Astronomie Vienna   (Austria)

^c UNIVERSITY OF WISCONSIN MADISON   (United States)

^d NORTHERN ARIZONA UNIVERSITY   (United States)

^e SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^f ODESSA NATIONAL UNIVERSITY   (Ukraine)

^g PERTH OBSERVATORY   (Australia)

Author keywords

Stars: chemically peculiar; Stars: individual: HR 8097; Stars: oscillations

Indexed keywords

GEOMETRICAL OPTICS; STARS;

HIGH SPEED; MODE SPECTRUM; NEW HIGH; P MODES; P-MODES; PHOTOMETRICS; STAR OSCILLATIONS; STAR: INDIVIDUAL: HR 8097; STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: PROXIMA CENTAURI;

LUMINANCE;

EID: 0000352145     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/282.1.243     Document Type: Article

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