Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 104
... dwarf PG 1159-035 , and the DBV white dwarfs GD 358 and PG 1115 + 158 to determine their internal structure in ... dwarf ( DAV ) stars . In spite of the relatively small number of observable modes in the DAV white dwarfs , several of ...
... dwarf PG 1159-035 , and the DBV white dwarfs GD 358 and PG 1115 + 158 to determine their internal structure in ... dwarf ( DAV ) stars . In spite of the relatively small number of observable modes in the DAV white dwarfs , several of ...
Page 209
... dwarf mass in Mo ' and 132 is the white dwarf's magnetic moment in units of 1032 G cm3 . For disk accretion , the magnetospheric radius should be slightly smaller ; theoretical estimates suggest Rmag≈0.5 R ( Lamb 1988 ) . The release ...
... dwarf mass in Mo ' and 132 is the white dwarf's magnetic moment in units of 1032 G cm3 . For disk accretion , the magnetospheric radius should be slightly smaller ; theoretical estimates suggest Rmag≈0.5 R ( Lamb 1988 ) . The release ...
Page 858
... Dwarf novae are close , interacting binary systems consisting of a white dwarf and a K or M main - sequence star . The secondary star fills its Roche lobe and is transferring mass to the white dwarf through the inner Lagrangian point ...
... Dwarf novae are close , interacting binary systems consisting of a white dwarf and a K or M main - sequence star . The secondary star fills its Roche lobe and is transferring mass to the white dwarf through the inner Lagrangian point ...
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abundance additional analysis appear associations assumed Astronomical average binary blue bright calibration catalog central clouds cluster color compared correction derived detection determined discussed distance distribution dwarf eclipse effects emission errors estimate et al evidence evolution field Figure flux frame function galaxies giants given groups included increase indices less light limit lines luminosity magnitude mass mean measured MNRAS nebulae noted objects observations obtained optical orbital PASP period phase photometric pixels position possible present probably quasars range ratio reduced reference region relation relative rotation sample scale scatter secondary shown similar sources spectral spectrum standard stars stellar stellar winds suggests surface survey Table telescope temperature tion University values variability velocity wavelength X-ray