Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 590
1 106 : 590-599 , 1994 June Analyses of Archival Data for Cool Dwarfs . III . The Choice and Application of Analysis Procedures BENJAMIN J. TAYLOR Physics and Astronomy Department , ESC , Brigham Young University , Provo , Utah 84602 ...
1 106 : 590-599 , 1994 June Analyses of Archival Data for Cool Dwarfs . III . The Choice and Application of Analysis Procedures BENJAMIN J. TAYLOR Physics and Astronomy Department , ESC , Brigham Young University , Provo , Utah 84602 ...
Page 606
... Analysis A and +0.005 for Analysis B. Clearly nothing essential is changed . Before deciding how far to trust this result , it is probably wise to visualize ways in which it might be challenged or altered in the future . The first ...
... Analysis A and +0.005 for Analysis B. Clearly nothing essential is changed . Before deciding how far to trust this result , it is probably wise to visualize ways in which it might be challenged or altered in the future . The first ...
Page 704
... analysis which yields averaged values of [ Fe / H ] for almost all of these stars . Paper IV ( Taylor 1994d ) uses some of these data in a discussion of the Hyades and Coma clusters . Paper R ( Taylor 1994e ) will consider the status of ...
... analysis which yields averaged values of [ Fe / H ] for almost all of these stars . Paper IV ( Taylor 1994d ) uses some of these data in a discussion of the Hyades and Coma clusters . Paper R ( Taylor 1994e ) will consider the status of ...
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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