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Radial and nonradial periods and growth rates of an AI Velorum model [electronic resource].

Published
Washington, D.C. : United States. Dept. of Energy, 1992.
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy.
Physical Description
Pages: (5 pages) : digital, PDF file
Additional Creators
Los Alamos National Laboratory, United States. Department of Energy, and United States. Department of Energy. Office of Scientific and Technical Information
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Summary
Walraven, Walraven, and Balona recently discovered several new periodicities in addition to the well-known fundamental and first overtone periods of the high-amplitude δ Scuti star AI Velorum. Linear nonadiabatic pulsation calculations were performed for an AI Velorum model of mass 1.96 M{sub {circle dot}}, 24.05 L{sub {circle dot}}, and T{sub eff}7566 K for the radial and low-degree nonradial modes to help verify the tentative identifications made by Walraven, et al. Comparison of the calculated periods with the observations suggests some alternatives to the identifications proposed by Walraven, et al.
Report Numbers
E 1.99:la-ur-92-861
E 1.99: conf-920184--3
conf-920184--3
la-ur-92-861
Subject(s)
Other Subject(s)
Note
Published through SciTech Connect.
01/01/1992.
"la-ur-92-861"
" conf-920184--3"
"DE92011369"
International Astronomical Union (IAU) meeting, Mito (Japan), 6-10 Jan 1992.
Guzik, J.A.
Funding Information
W-7405-ENG-36
View MARC record | catkey: 13825624