Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 448
... relation to metallicity for the Hyades , Coma , and field stars . In practice , this means that the safest way to ... relation between spectral types and B - V . The Nicolet ( 1978 ) Hyades values of B - V were again adopted . From a ...
... relation to metallicity for the Hyades , Coma , and field stars . In practice , this means that the safest way to ... relation between spectral types and B - V . The Nicolet ( 1978 ) Hyades values of B - V were again adopted . From a ...
Page 456
... relation was being derived , AM , was now obtained from a comparison to either the composite Heckmann - Johnson relation or a relation derived from Eggen's ( 1982 ) results [ see Table 5 , Eq . ( T9 ) ] . The scatter around these relations ...
... relation was being derived , AM , was now obtained from a comparison to either the composite Heckmann - Johnson relation or a relation derived from Eggen's ( 1982 ) results [ see Table 5 , Eq . ( T9 ) ] . The scatter around these relations ...
Page 479
... relation should be valid in the mean in view of the P - L relation exhibited by the variable stars . We assume that this is indeed the case and write the P√p = Q relation as Mbol - 3.33 log P - 1.67 log M / M - 10 log Teff + Mbol + 10 ...
... relation should be valid in the mean in view of the P - L relation exhibited by the variable stars . We assume that this is indeed the case and write the P√p = Q relation as Mbol - 3.33 log P - 1.67 log M / M - 10 log Teff + Mbol + 10 ...
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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