Observations of galactic WC + O binary systems: HD 97152 and HD 152270

Details Observations of galactic WC + O binary systems: HD 97152 and HD 152270 Observations of galactic WC + O binary systems: HD 97152 and HD 152270

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281a.193a&link_type=abstract

In ESA, A Decade of UV Astronomy with the IUE Satellite, Volume 1 p 193-195 (SEE N89-10682 01-89)

Astronomy and Astrophysics

Astronomy

1

Binary Stars, Iue, Spaceborne Astronomy, Ultraviolet Astronomy, Ultraviolet Spectra, Wolf-Rayet Stars, Emission Spectra, Stellar Orbits

Scientific paper

The IUE observations of the Wolf-Rayet binary systems HD 97152 and HD
152270 are presented. Both systems contain a WC7 component, and both
have relatively small orbital inclinations. Weak atmospheric eclipses at
emission line wavelengths are detected in HD 97152, the system for which
a more suitable phase coverage is available.

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