Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 198
... ratio is required . It may be obtained from a solution of the light curve if one is available . In nearly all real cases , the binary spectrum is too complicated ( see Figs . 3 and 4 ) for a direct determination of the ratio from ...
... ratio is required . It may be obtained from a solution of the light curve if one is available . In nearly all real cases , the binary spectrum is too complicated ( see Figs . 3 and 4 ) for a direct determination of the ratio from ...
Page 360
... ratio . In this and subsequent figures only the central 160x160 pixels are plotted to avoid marked cosmetic ... ratio of o Dra to e Eri at the 36 ° position angle . The ratio procedure has heavily reduced both the skirt of the psf and ...
... ratio . In this and subsequent figures only the central 160x160 pixels are plotted to avoid marked cosmetic ... ratio of o Dra to e Eri at the 36 ° position angle . The ratio procedure has heavily reduced both the skirt of the psf and ...
Page 481
... ratio relation , giving a mass ratio ( MRD / M wD ) of 0.20 for BZ UMa . The short period , long outburst interval , and small mass ratio support the suggestion of BZ UMa being in the SU Ursae Majoris subclass of dwarf novae . 4. 106 ...
... ratio relation , giving a mass ratio ( MRD / M wD ) of 0.20 for BZ UMa . The short period , long outburst interval , and small mass ratio support the suggestion of BZ UMa being in the SU Ursae Majoris subclass of dwarf novae . 4. 106 ...
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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