New solution to viscous evolution of accretion disks in binary systems

Details New solution to viscous evolution of accretion disks in binary systems New solution to viscous evolution of accretion disks in binary systems

Publishing date

Jul 2008

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008a%26a...485..153l&link_type=abstract

Journals

Astronomy and Astrophysics, Volume 485, Issue 1, 2008, pp.153-153

Science

Astronomy and Astrophysics

Field

Astrophysics

Additional info 3

Errata, Addenda, Accretion, Accretion Disks, Stars: Binaries: Close, Stars: Novae, Cataclysmic Variables, X-Rays: Bursts

Type

Scientific paper

Abstract

We find several mistakes that affect the physical precision of some of our formulae but not the principal conclusions of our work (A&A 356, 363-372 (2000)). The derived law of accretion disk evolution is correct, although some numerical factors in the resulting expressions for physical parameters require an update. The rest of the corrections apply to the notations in the equations.

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