An accurate geometric distance to the compact binary SS Cygni vindicates accretion disc theory

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An accurate geometric distance to the compact binary SS Cygni vindicates accretion disc theory

Dwarf novae are white dwarfs accreting matter from a nearby red dwarf companion. Their regular outbursts are explained by a thermal-viscous instability in the accretion disc, described by the disc instability model that has since been successfully extended to other accreting systems. However, the pr...

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Bibliographic Details
Main Authors:	Miller-Jones, James, Sivakoff, G., Knigge, C., Koerding, E., Templeton, M., Waagen, E.
Format:	Journal Article
Published:	The American Association for the Advancement of Science 2013
Online Access:	http://www.sciencemag.org/content/340/6135/950 http://hdl.handle.net/20.500.11937/47140

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