Absolute magnitude in the K band of carbon stars
The relationship between the absolute magnitude in the K band and the IRAS color index of (12)-(25) was derived for carbon stars in the solar neighborhood by kinematical analyses of the radial-velocity data and the newly published proper-motion data in the ACRS catalog. The mean absolute magnitude i...
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Veröffentlicht in: | Publications of the Astronomical Society of Japan 1993-08, Vol.45 (4), p.587-593 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | The relationship between the absolute magnitude in the K band and the IRAS color index of (12)-(25) was derived for carbon stars in the solar neighborhood by kinematical analyses of the radial-velocity data and the newly published proper-motion data in the ACRS catalog. The mean absolute magnitude in the K band of carbon stars varies from -8.0 to -8.6 with increases of 0.1 to 0.6 in (12)-(25). This tendency indicates that the more luminous carbon stars have a thicker circumstellar dust shell. |
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ISSN: | 0004-6264 |