Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 132
... determined in the standard way . Per , The following comparison stars were used : for HR 1034 ( HD 21278 , V = 4.98 ... determined from Zeta Tau using extinction coefficient determined from Psi Per 5. ANALYSIS It was immediately apparent ...
... determined in the standard way . Per , The following comparison stars were used : for HR 1034 ( HD 21278 , V = 4.98 ... determined from Zeta Tau using extinction coefficient determined from Psi Per 5. ANALYSIS It was immediately apparent ...
Page 242
... determined spectral classes from the literature are a possibility , since most of these types were presumably determined from double - lined spectroscopic binaries outside of eclipse , against the com- peting light of the primary ...
... determined spectral classes from the literature are a possibility , since most of these types were presumably determined from double - lined spectroscopic binaries outside of eclipse , against the com- peting light of the primary ...
Page 739
... determined . This approach was used to determine the brightness peaks of the lobes and ansae . The analysis is complicated slightly by the fact that their radial profiles are much broader than that of a star , and they are not ...
... determined . This approach was used to determine the brightness peaks of the lobes and ansae . The analysis is complicated slightly by the fact that their radial profiles are much broader than that of a star , and they are not ...
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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