Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000newar..44...21d&link_type=abstract
New Astronomy Reviews, Volume 44, Issue 1-2, p. 21-26.
Astronomy and Astrophysics
Astronomy
20
Scientific paper
The concept of an `effective' Eddington limit as a lower bound on the system luminosity required for mass loss to be radiation pressure driven is discussed and shown to fall in the interesting regime for high-state non-magnetic CV (nMCV). The results of recent hydrodynamical models of radiation-driven disk winds (Proga et al. 1998, Proga 1999) are summarised. Mass loss rates predicted by these models are then compared with observational constraints. It is shown that either mass accretion rates in high-state nMCV are a factor of 2-3 larger than presently supposed or that radiation pressure alone is not quite sufficient to drive the observed hypersonic flows.
Drew Janet E.
Proga Daniel
No associations
LandOfFree
Radiation-driven accretion disk winds does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Radiation-driven accretion disk winds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiation-driven accretion disk winds will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1625507