Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 452
... given for 417 of these stars in a catalog at the end of this paper . ( Readers who are interested only in these data should proceed directly to Sec . 6 and Table 8. ) The derived temperatures are based largely on a calibration given by ...
... given for 417 of these stars in a catalog at the end of this paper . ( Readers who are interested only in these data should proceed directly to Sec . 6 and Table 8. ) The derived temperatures are based largely on a calibration given by ...
Page 683
... Given a few determinations of the occurrence of a periodic event spanning a large interval of time , one can hope to make detailed determinations of the period and its behavior with time . This is accomplished by obtaining the correct ...
... Given a few determinations of the occurrence of a periodic event spanning a large interval of time , one can hope to make detailed determinations of the period and its behavior with time . This is accomplished by obtaining the correct ...
Page 704
... given in Table 2 , which is found in the four pages at the very end of the paper . For each star listed , Table 2 includes mean values and rms errors for [ Fe / H ] . Effective numbers of degrees of freedom ( values of v ) are also given ...
... given in Table 2 , which is found in the four pages at the very end of the paper . For each star listed , Table 2 includes mean values and rms errors for [ Fe / H ] . Effective numbers of degrees of freedom ( values of v ) are also given ...
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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