Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 436
... calibration reproduces satisfactorily the infrared temperature scale of Bell and Gustafsson ( 1989 ) . It is shown that Osborn's ( 1979 ) calibration underestimates the effective temperatures of K giants by ~ 170 K and those of late ...
... calibration reproduces satisfactorily the infrared temperature scale of Bell and Gustafsson ( 1989 ) . It is shown that Osborn's ( 1979 ) calibration underestimates the effective temperatures of K giants by ~ 170 K and those of late ...
Page 452
... calibration presented in a previous paper is used in this paper to derive temperatures for FGK stars near the main sequence . The calibration is checked against published counterparts , and it is found that previous calibrations have ...
... calibration presented in a previous paper is used in this paper to derive temperatures for FGK stars near the main sequence . The calibration is checked against published counterparts , and it is found that previous calibrations have ...
Page 468
... calibration . Compare this figure with Fig . 2 and consult Table 2 for more information . -10 -5 ap ( VI ) FIG . 5 ... Calibration As we said before , a need of a calibration similar to that developed in previous sections exists for the ...
... calibration . Compare this figure with Fig . 2 and consult Table 2 for more information . -10 -5 ap ( VI ) FIG . 5 ... Calibration As we said before , a need of a calibration similar to that developed in previous sections exists for the ...
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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