Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 125
... variability behavior of a quasar . This in turn will include at least two factors : time scale and amplitude , and these may not be separable . The amplitude and time scale of the variability exhibited by a quasar will also show a ...
... variability behavior of a quasar . This in turn will include at least two factors : time scale and amplitude , and these may not be separable . The amplitude and time scale of the variability exhibited by a quasar will also show a ...
Page 373
... variability increases during secondary eclipse . Variability decreases as primary eclipse progresses . Primary significance of the regions A and B ( Fig . 4 ) over a number of orbital cycles . 1 3.2 Eclipse Phase The polarimetric ...
... variability increases during secondary eclipse . Variability decreases as primary eclipse progresses . Primary significance of the regions A and B ( Fig . 4 ) over a number of orbital cycles . 1 3.2 Eclipse Phase The polarimetric ...
Page 373
... variability increases during secondary eclipse . Variability decreases as primary eclipse progresses . -ד significance of the regions A and B ( Fig . 4 ) over a number of orbital cycles . 3.2 Eclipse Phase The polarimetric variability ...
... variability increases during secondary eclipse . Variability decreases as primary eclipse progresses . -ד significance of the regions A and B ( Fig . 4 ) over a number of orbital cycles . 3.2 Eclipse Phase The polarimetric variability ...
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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