A comment on the nature of O-type runaway stars

Details A comment on the nature of O-type runaway stars A comment on the nature of O-type runaway stars

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....86...68p&link_type=abstract

Astronomy and Astrophysics, vol. 86, no. 1-2, June 1980, p. 68-71.

Astronomy and Astrophysics

Astrophysics

14

Early Stars, O Stars, Star Distribution, Data Processing, Stellar Motions, Stellar Spectra

Scientific paper

The characteristics of O-type runaway stars are compared with those of
normal, low-velocity O stars, in order to test the hypothesis that the
runaway stars are members of the Old Disk Population. No evidence to
support the hypothesis is found. The strong concentration to the
galactic plane shows that they are Extreme Population I stars.

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