Origins and ages of X-ray-luminous dwarf M stars

Details Origins and ages of X-ray-luminous dwarf M stars Origins and ages of X-ray-luminous dwarf M stars

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...273..702j&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 273, Oct. 15, 1983, p. 702-708.

Other

32

Dwarf Stars, Late Stars, M Stars, Stellar Evolution, Stellar Luminosity, X Ray Sources, Hertzsprung-Russell Diagram, Interstellar Matter, Mass To Light Ratios, Stellar Motions

Scientific paper

The nearby M dwarfs for which published X-ray data are available are assembled and examined for kinematical and other evidence of their age. Those with the highest order of X-ray luminosity are presumably young, but subsets of them fall kinematically into old disk as well as young disk populations. The youthful "old disk" M dwarfs may have formed recently in the interstellar high-velocity clouds or intermediate-velocity clouds from which they derive their kinematical properties.

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