Al. Desetangs et al., DUST DISTRIBUTION IN RADIATION PRESSURE OUTFLOW - APPLICATION TO THE BD-DEGREES-643 DISK(31), Astronomy and astrophysics (Berlin), 339(2), 1998, pp. 477-482
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+31 degrees 633 can be explained by this simple model,
provided that the ambient gas of the surrounding cluster IC 348 has a
density rho similar to 10(4) cm(-3) The dust is probably produced with
in 2300 AU from the central binary star.