Ultraviolet observations of circumstellar matter in Algol type binary systems

Details Ultraviolet observations of circumstellar matter in Algol type binary systems Ultraviolet observations of circumstellar matter in Algol type binary systems

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2349..387p&link_type=abstract

In NASA. Goddard Space Flight Center Future of Ultraviolet Astronomy Based on Six Years of IUE Res. p 387-390 (SEE N85-20961 1

Astronomy and Astrophysics

Astronomy

Absorption Spectra, Far Ultraviolet Radiation, Iue, Line Spectra, Stellar Envelopes, Far Uv Spectroscopic Explorer, Resonance Lines, Ultraviolet Spectroscopy

Scientific paper

Properties of four components to the circumstellar matter in Algol type interacting binary systems which have been investigated with the aid of timed high resolution IUE observations are discussed. Included are the high temperature accretion region, gas stream, restricted domains of material outflow, and the general wind. In particular, the authors comment on the geometrical distribution in the system, physical conditions, flow patterns, and stability. CX Dra serves as an illustrative example and a model for the circumstellar matter in this system is presented.

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