Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 228
... evidence . Some additional evidence already exists in the X - ray pulses . The binary inclination is very high , and it therefore seems very likely that the accreting pole is carried fully around the limb of the star . Yet the pulsed ...
... evidence . Some additional evidence already exists in the X - ray pulses . The binary inclination is very high , and it therefore seems very likely that the accreting pole is carried fully around the limb of the star . Yet the pulsed ...
Page 506
... evidence in the observed CO ther- mal emission of massive nebulae ( e.g. , Knapp et al . 1982 ) as would be expected if the envelopes were significantly accel- erated beyond their original AGB velocity , with the excep- tion of the very ...
... evidence in the observed CO ther- mal emission of massive nebulae ( e.g. , Knapp et al . 1982 ) as would be expected if the envelopes were significantly accel- erated beyond their original AGB velocity , with the excep- tion of the very ...
Page 624
... evidence that the continuum temperatures are systematically lower than forbidden - line temperatures ; he estimates that the bulk of evidence seems to favor nearly equal continuum and forbidden - line temperatures ; and Shaver et al ...
... evidence that the continuum temperatures are systematically lower than forbidden - line temperatures ; he estimates that the bulk of evidence seems to favor nearly equal continuum and forbidden - line temperatures ; and Shaver et al ...
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absorption abundance accretion analysis asteroids 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 pixel 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 stellar winds subgiant survey Table telescope temperature tion turnoff values variability wavelength white dwarf width X-ray XX Vir