The spectra of two new intermediate helium stars

Details The spectra of two new intermediate helium stars The spectra of two new intermediate helium stars

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...250..701d&link_type=abstract

Astrophysical Journal, Part 1, vol. 250, Nov. 15, 1981, p. 701-703. Research supported by the Louisiana State University, South

Other

4

B Stars, Early Stars, Helium, O Stars, Stellar Spectra, Hydrogen, Iue, Star Clusters, Ultraviolet Spectra

Scientific paper

The stars designated as LSS 2394 and LS II + 36 deg 37 in the Case-Hamburg Luminous Stars surveys are found to be intermediate helium stars. The environment and spectrum of LSS 2394 (CPD -62 2124) appear to be quite similar to those of Sigma Ori E in a number of respects, including close proximity to two other OB stars, membership in a rich O association, spectrum variability, rapid rotation, and broad H-alpha emission wings. A low-resolution IUE spectrum for this star is presented and discussed.

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