Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 154
... surface of a distorted binary star . It is shown that neither series is particularly accurate for very distorted ... surface ; otherwise , the material would " run downhill " and change the star's shape . If the stars are assumed to be ...
... surface of a distorted binary star . It is shown that neither series is particularly accurate for very distorted ... surface ; otherwise , the material would " run downhill " and change the star's shape . If the stars are assumed to be ...
Page 430
... surface , as shown in Fig . 4 ( b ) . Upon heating by sunlight , surface volatiles sublimate , entraining dust particles in the gas flow . The largest dust particles will be too heavy to reach escape speed and will accumulate on the surface ...
... surface , as shown in Fig . 4 ( b ) . Upon heating by sunlight , surface volatiles sublimate , entraining dust particles in the gas flow . The largest dust particles will be too heavy to reach escape speed and will accumulate on the surface ...
Page 602
... surface abundances decrease . For cluster stars in particular , the surface metallicities of giants and dwarfs would then differ , and the surface metallicities of giants would vary along the giant branch . In addition , there would be ...
... surface abundances decrease . For cluster stars in particular , the surface metallicities of giants and dwarfs would then differ , and the surface metallicities of giants would vary along the giant branch . In addition , there would be ...
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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