Absolute magnitudes of late-type stars

Details Absolute magnitudes of late-type stars Absolute magnitudes of late-type stars

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119...65m&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

5

Carbon Stars, Cool Stars, Late Stars, M Stars, Stellar Luminosity, Stellar Magnitude, Calibrating, Maximum Likelihood Estimates, Statistical Analysis, Stellar Motions

Scientific paper

The improved calibration of absolute magnitude versus spectral type and luminosity class is presented for carbon stars and for K- to M-type giants. It is based on the recent results estimated by applying the maximum-likelihood method and other statistical methods to the homogeneous kinematical data including the proper motions in the AGK3 system.

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