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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absorption abundance accretion analysis asteroids astrometry Astronomical Society binary bright calibration catalog central star chromospheric clouds color comets correction derived detection detector diagram disk distribution eclipse emission errors estimate evolution expansion velocities Fe/H field flux frame function galactic galaxies GCLF giant branch globular clusters H II regions Hyades indices infrared ionized km s¹ light curve lines luminosity magnitude main sequence main-sequence mass measured MNRAS objects observations Observatory obtained open clusters optical orbital parameters PASP period phase photometric pixels planetary nebulae plotted quasars radial velocities radius range ratio red giants reddening redshift region residuals rotation sample scale scatter secondary solar sources spectral type spectroscopic spectrum standard stellar subgiant survey Table telescope temperature tion turnoff values variability wavelength white dwarf width X-ray XX Vir