Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 218
... period , visible in U light , as well as QPOS in the lowfrequency wing of the primary signal . The various reports of QPOS ( Patterson 1981 ; Mazeh et al . 1985 ; Patterson 1991 ) suggest that the QPO period is longer in outburst than ...
... period , visible in U light , as well as QPOS in the lowfrequency wing of the primary signal . The various reports of QPOS ( Patterson 1981 ; Mazeh et al . 1985 ; Patterson 1991 ) suggest that the QPO period is longer in outburst than ...
Page 479
... period of pulsation . The equation predicts Teff = 6450 K at log P = 0 and Teff = 5300 K at log P = 1.5 . The 6450 K value is based on our Teff values of XX Vir and V716 Oph . We have inferred the Teff of the longer - period stars from ...
... period of pulsation . The equation predicts Teff = 6450 K at log P = 0 and Teff = 5300 K at log P = 1.5 . The 6450 K value is based on our Teff values of XX Vir and V716 Oph . We have inferred the Teff of the longer - period stars from ...
Page 481
... period has led to suggestions that this object is intermediate to the WZ Sagittae and U Gem classes ( Wenzel 1982 ) . Szkody and Feinswog ( 1988 ) found an infrared sinusoidal variation with a period of 107 ± 11 min . Assuming this is ...
... period has led to suggestions that this object is intermediate to the WZ Sagittae and U Gem classes ( Wenzel 1982 ) . Szkody and Feinswog ( 1988 ) found an infrared sinusoidal variation with a period of 107 ± 11 min . Assuming this is ...
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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