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Title:
Bolometric luminosities and colors for K and M dwarfs and the subluminous stars of the halo
Authors:
Greenstein, Jesse L.
Affiliation:
AA(Palomar Observatory; California Institute of Technology, Pasadena)
Publication:
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 101, Sept. 1989, p. 787-810. (PASP Homepage)
Publication Date:
09/1989
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
ESCAPE VELOCITY, HALOS, MAIN SEQUENCE STARS, STELLAR COLOR, STELLAR LUMINOSITY, SUBDWARF STARS, BOLOMETERS, COLOR-COLOR DIAGRAM, ENERGY DISTRIBUTION, HERTZSPRUNG-RUSSELL DIAGRAM, INFRARED PHOTOMETRY, TABLES (DATA), WEIGHTING FUNCTIONS
DOI:
10.1086/132500
Bibliographic Code:
1989PASP..101..787G

Abstract

The H-R diagrams of dM, sdK, and sdM proper-motion stars are examined. A method for integrating energy distributions using discrete weights is proposed. The bolometric corrections are assessed at various wavelengths and a method for obtaining luminosities even if a star lacks IR data is presented. The color-luminosity diagrams suggest that high-velocity, low-metallicity stars of the halo are subluminous. It is found that the apparent cutoff in the halo is a bolometric magnitude of about 12 m.

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