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Spectrum of the novalike binary UX Ursae Majoris

Journal Article · · Sov. Astron. Lett. (Engl. Transl.); (United States)
OSTI ID:6100475
Spectroscopy of the novalike binary UX UMa with the 6-m telescope during 1977--1980 is reported. Analysis of all available data indicates that the time evolution of the spectrum can be understood if the system contains not only the usual accretion disk but also an extended envelope. The object might prove to be an x-ray burster.
Research Organization:
Special Astrophysical Observatory, USSR Academy of Sciences, Nizhnii Arkhyz
OSTI ID:
6100475
Journal Information:
Sov. Astron. Lett. (Engl. Transl.); (United States), Journal Name: Sov. Astron. Lett. (Engl. Transl.); (United States) Vol. 11:4; ISSN SALED
Country of Publication:
United States
Language:
English

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Related Subjects

640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ACCRETION DISKS
BALMER LINES
BINARY STARS
COSMIC RAY SOURCES
COSMIC X-RAY SOURCES
ELECTROMAGNETIC RADIATION
ERUPTIVE VARIABLE STARS
HARD X RADIATION
IONIZING RADIATIONS
MASS TRANSFER
NOVAE
OSCILLATIONS
RADIATIONS
SPECTRA
STAR ACCRETION
STAR EVOLUTION
STARS
VARIABLE STARS
VISIBLE SPECTRA
X RADIATION