New solution to viscous evolution of accretion disks in binary systems
Sternberg Astronomical Institute, Moscow State University, Universitetskij pr. 13, 119992 Moscow, Russia e-mail: email@example.com
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.
Key words: errata, addenda / accretion, accretion disks / stars: binaries: close / stars: novae, cataclysmic variables / X-rays: bursts
© ESO, 2008