Properties of components of the UZ Librae system

Details Properties of components of the UZ Librae system Properties of components of the UZ Librae system

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...223..172g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 223, no. 1-2, Oct. 1989, p. 172-178.

Astronomy and Astrophysics

Astrophysics

13

Binary Stars, Giant Stars, K Stars, Stellar Spectrophotometry, Black Body Radiation, Emission Spectra, Iue, Photosphere, Stellar Rotation, Ultraviolet Spectra

Scientific paper

A reanalysis is conducted of the available photometric and spectroscopic data for the K-giant UZ Librae, including recent uvby photometry. The rotational period thus derived is close to, but not identical with the orbital period. Attention is given to UV spectra taken at different orbital/rotational phases. It is concluded that the overall properties of the system fit the evolutionary scenario of a coalescing binary described by Webbink (1976).

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