Spectral types for faint blue stars near the galactic anticenter

Details Spectral types for faint blue stars near the galactic anticenter Spectral types for faint blue stars near the galactic anticenter

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aj.....84..534c&link_type=abstract

Astronomical Journal, vol. 84, Apr. 1979, p. 534-537. Research supported by the City University of New York.

Astronomy and Astrophysics

Astronomy

18

Astronomical Spectroscopy, Early Stars, Milky Way Galaxy, Stellar Spectra, Radial Velocity, Stellar Luminosity, Stellar Magnitude, Velocity Measurement

Scientific paper

Spectral types are given for 49 blue stars whose photometry places them at large distances from the galactic center. The majority of the stars appear to be population I objects, 15-25 kpc from the center. Most of the remainder are relatively nearby blue horizontal branch stars or hot subdwarfs. One apparently normal O5 V star would be more than 50 kpc from the galactic center if it has the luminosity indicated by its spectrum.

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