Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 201
... Bright Stars in Omega Centauri and the Type II Cepheid ST Puppis GUILLERMO GONZALEZ Thesis work conducted at : Department of Astronomy , University of Washington Current address : Department of Astronomy and McDonald Observatory ...
... Bright Stars in Omega Centauri and the Type II Cepheid ST Puppis GUILLERMO GONZALEZ Thesis work conducted at : Department of Astronomy , University of Washington Current address : Department of Astronomy and McDonald Observatory ...
Page 267
... bright stars with comparatively large photometric errors are also within the profiles of still brighter stars . These facts warn us that individual objects displaying unusual colors must be examined visually before they are assumed to ...
... bright stars with comparatively large photometric errors are also within the profiles of still brighter stars . These facts warn us that individual objects displaying unusual colors must be examined visually before they are assumed to ...
Page 272
... bright ( V < 15.5 ) giants , whose flux - weighted mean apparent magnitude is 14.42 . If the giant branch as a whole is shifted to the blue by 0.1 mag ( 10 % ) compared to its outer - cluster counterpart , the 70 bright giants produce ...
... bright ( V < 15.5 ) giants , whose flux - weighted mean apparent magnitude is 14.42 . If the giant branch as a whole is shifted to the blue by 0.1 mag ( 10 % ) compared to its outer - cluster counterpart , the 70 bright giants produce ...
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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