Dust distribution in radiation pressure outflow. Application to the BD+31d643 disk
Etangs, A. Lecavelier des · Vidal-Madjar, A. · Ferlet, R.
Original · EN
The radial distribution of dust has been calculated in outflows driven by radiation pressure in which the gas drag is taken into account. It is shown that the dust distribution in the newly discovered candidate disk around BD+31d643 can be explained by this simple model, provided that the ambient gas of the surrounding cluster IC 348 has a density ρ 10⁴ cm⁻³. The dust is probably produced within 2300 AU from the central binary star.
English translation
This paper has no Arabic translation yet. Be the first: it takes a few seconds, and the result is stored for every future reader.