The distribution of luminous stars at (l,b) = (245 deg, 0 deg) in Puppis

Details The distribution of luminous stars at (l,b) = (245 deg, 0 deg) in Puppis The distribution of luminous stars at (l,b) = (245 deg, 0 deg) in Puppis

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.211..235r&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 211, Nov. 1, 1984, p. 235-241. Research supported by th

Astronomy and Astrophysics

Astronomy

13

Astrometry, B Stars, O Stars, Star Distribution, Density Distribution, Interstellar Extinction, Stellar Parallax

Scientific paper

Munch (1951, 1954) drew attention to the presence of a concentration of faint OB stars along the galactic equator at l = 245 deg in Puppis. The distribution of OB stars in this field has subsequently been studied by a number of workers. It has now been found that the distribution of OB stars in Puppis is not well established. The present investigation has, therefore, the objective to reexamine all available spectroscopic and photometric data on these OB stars in a systematic fashion, utilizing the method of spectroscopic parallaxes rather than H-beta photometry or ZAMS fitting. Attention is given to interstellar extinction, stellar distribution perpendicular to the Galactic plane, and the stellar density distribution.

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