Emerging picture of accretion shocks in detached binaries

Details Emerging picture of accretion shocks in detached binaries Emerging picture of accretion shocks in detached binaries

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.263..439a&link_type=abstract

In ESA Proceedings of an International Symposium on New Insights in Astrophysics. Eight Years of UV Astronomy with IUE p 439-44

Astronomy and Astrophysics

Astrophysics

2

Eclipsing Binary Stars, Stellar Mass Accretion, Stellar Spectra, Stellar Winds, Iue, Line Spectra, Stellar Models, Ultraviolet Spectra

Scientific paper

Research over the last few years, principally with the IUE observatory, has clearly demonstrated the existence of shock interactions and accretion in detached binaries like the ζ Aurigae type systems. The authors present preliminary results of the N V lines in these systems, including the evidence for a reverse P-Cygni profile in ζ Aur and 22 Vul. They examine differences in observable parameters among the systems in the light of their current research.

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