PROBLEMS IN THE TEMPERATURE CLASSIFICATION OF THE RED GIANT STARS
Effective temperatures determined by Tsuji by the infrared-flux method were shown by him to remain nearly constant in the range M0 to M2. It is easily shown that this is not due to any luminosity effect in the spectral types. Rather, revised MK types based primarily on TiO band strengths in this ran...
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Veröffentlicht in: | Publications of the Astronomical Society of the Pacific 1982-04, Vol.94 (558), p.299-303 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | Effective temperatures determined by Tsuji by the infrared-flux method were shown by him to remain nearly constant in the range M0 to M2. It is easily shown that this is not due to any luminosity effect in the spectral types. Rather, revised MK types based primarily on TiO band strengths in this range are shown to be more sensitive to temperature changes than are the commonly used color indices. |
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ISSN: | 0004-6280 1538-3873 |
DOI: | 10.1086/130980 |