Absolute magnitudes of late-type stars

descriptionPublicationkeyboard_double_arrow_right Article , Part of book or chapter of book 01 Jan 1986 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics and Space Science, volume 119, pages 65-68 (issn: 0004-640X, eissn: 1572-946X,

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Authors: Takao Mikami;

doi: 10.1007/bf00648814 , 10.1007/978-94-009-4630-9_14

Absolute magnitudes of late-type stars

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Abstract

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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University of Tokyo
Japan

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