Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 14
... probably the record for any active star . The galloping giant . Ap91 chronicled the first 90 years of rapid evolution of FG Sagittae . Quite unexpectedly , in August - September 1992 , it faded back from V = 9 to V = 13 , almost as ...
... probably the record for any active star . The galloping giant . Ap91 chronicled the first 90 years of rapid evolution of FG Sagittae . Quite unexpectedly , in August - September 1992 , it faded back from V = 9 to V = 13 , almost as ...
Page 228
... probably due to photoelectric absorption in a structure which moves around the white dwarf with the binary period . What structure is this ? Most of the dips occur ~ 0.2 cycles before inferior conjunction of the secondary ; this is when ...
... probably due to photoelectric absorption in a structure which moves around the white dwarf with the binary period . What structure is this ? Most of the dips occur ~ 0.2 cycles before inferior conjunction of the secondary ; this is when ...
Page 792
cated systems . Since cosmic rays are probably accelerated with substantial efficiencies in SNRs , their dynamical contributions must be included there , and probably elsewhere when strong shocks are present . However , the method has ...
cated systems . Since cosmic rays are probably accelerated with substantial efficiencies in SNRs , their dynamical contributions must be included there , and probably elsewhere when strong shocks are present . However , the method has ...
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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