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 and used if possible , and transformation coefficients were determined in the standard way . -1.85 O The following comparison stars were used : for & Per , HR 1034 ( HD 21278 , V = 4.98 , ( B - V ) = - 0.09 , B5 V ) and HR ...
... determined and used if possible , and transformation coefficients were determined in the standard way . -1.85 O The following comparison stars were used : for & Per , HR 1034 ( HD 21278 , V = 4.98 , ( B - V ) = - 0.09 , B5 V ) and HR ...
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 competing 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 competing light of the primary ...
Page 818
... determined from spectral indices . * Determined from Bessel and Brett's ( 1988 ) sp . type vs. ( V - I ) , relation . " Determined from Leggett's ( 1992 ) sp . type vs. ( V - I ) , relation . < 1.5 2.5 < 1.5 < 1.5 2.5 3.0 3.5 5.0 < 1.5 ...
... determined from spectral indices . * Determined from Bessel and Brett's ( 1988 ) sp . type vs. ( V - I ) , relation . " Determined from Leggett's ( 1992 ) sp . type vs. ( V - I ) , relation . < 1.5 2.5 < 1.5 < 1.5 2.5 3.0 3.5 5.0 < 1.5 ...
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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