MU Sagittarii and Beta Lyrae: Combined IUE/Voyager observations

Details MU Sagittarii and Beta Lyrae: Combined IUE/Voyager observations MU Sagittarii and Beta Lyrae: Combined IUE/Voyager observations

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2349..424p&link_type=abstract

In NASA. Goddard Space Flight Center Future of Ultraviolet Astronomy Based on Six Years of IUE Res. p 424-427 (SEE N85-20961 1

Astronomy and Astrophysics

Astronomy

Binary Stars, Iue, Oao 3, Supergiant Stars, Ultraviolet Spectra, Voyager Project, Hot Stars, Line Spectra, Stellar Envelopes, Stellar Motions

Scientific paper

A hot companion to the B8 Ia supergiant μ Sagittarii was discovered by observations with three satellites: Copernicus, IUE, and Voyager. The companion is probably a B2 V star, but could be as hot as B0. Voyager observations in the region 900 - 1700 Å have been started also for β Lyrae, and show that the disk-shaped secondary is the dominating source in the EUV.

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