Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 247
... eclipse were not smooth nor symmetric ( McKellar et al . 1959 ) . During ingress , only a few cases of line asymmetry were seen , with most observations not showing any clear structure ... eclipse at considerably 1982 ECLIPSE OF 31 CYGNI 247.
... eclipse were not smooth nor symmetric ( McKellar et al . 1959 ) . During ingress , only a few cases of line asymmetry were seen , with most observations not showing any clear structure ... eclipse at considerably 1982 ECLIPSE OF 31 CYGNI 247.
Page 373
... eclipse are indicated . 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 ...
... eclipse are indicated . 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 ...
Page 373
... eclipse are indicated . The polarimetric 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 ...
... eclipse are indicated . The polarimetric 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 ...
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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