Spectroscopy of five faint M dwarf stars near the north galactic pole

Details Spectroscopy of five faint M dwarf stars near the north galactic pole Spectroscopy of five faint M dwarf stars near the north galactic pole

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasp...87..885k&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 87, Dec. 1975, p. 885-889.

Astronomy and Astrophysics

Astronomy

8

Dwarf Stars, M Stars, Stellar Luminosity, Stellar Motions, Stellar Spectrophotometry, Late Stars, Luminous Intensity, Radial Velocity, Spectral Line Width

Scientific paper

Radial velocities and estimates of absolute magnitudes are presented for five M dwarfs selected from a proper-motion study of M stars near the north galactic pole by Murray and Sanduleak (1972). The derived mean distance and velocity dispersion are significantly larger than the corresponding quantities found by Murray and Sanduleak, but only a small sample limited to the earlier-type stars on their list was used in the present study.

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