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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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