UV and X-ray imaging of interacting binary systems

Details UV and X-ray imaging of interacting binary systems UV and X-ray imaging of interacting binary systems

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006pobeo..80..117k&link_type=abstract

Publications of the Astronomical Observatory of Belgrade, Vol. 80, p. 117-118

Astronomy and Astrophysics

Astronomy

Scientific paper

Multi-wavelength studies of many currently unresolved interacting binary systems have detected dramatic changes in the spectral distribution of the emission related to changes in accretion processes. These studies demonstrate that there are many aspects of accretion processes in general, and of wind accretion processes in particular, that are not yet understood. The key to further accretion studies is resolving a wide range of interacting binaries and studying their components and mass flows. I discuss current and future prospects for resolving a wide range of interacting binary systems.

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