MOCASSIN: 3D photoionisation and dust radiative transfer modelling of PNe

Details MOCASSIN: 3D photoionisation and dust radiative transfer modelling of PNe MOCASSIN: 3D photoionisation and dust radiative transfer modelling of PNe

2004-07-10

arxiv.org/abs/astro-ph/0407200v1

Astronomy and Astrophysics

Astrophysics

2 pages, 1 figure, proceedings to the ESO workshop on PNe beyond the Milky Way, Garching, May 2004

Scientific paper

We present the first 3D Monte Carlo photoionisation code to include a fully self-consistent treatment of dust radiative transfer (RT) within the photoionised region. This is the latest development of the recently published pure photoionisation code MOCASSIN (Ercolano et al., 2003a) and it is currently undergoing several benchmarking tests. The preliminary results of these tests are presented in these conference proceedings. The new code provides the ideal tool for the analysis of dusty ionised regions showing asymmetries and/or density and chemical inhomogeneities

Affiliated with

Also associated with

No associations

Rating

MOCASSIN: 3D photoionisation and dust radiative transfer modelling of PNe 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 MOCASSIN: 3D photoionisation and dust radiative transfer modelling of PNe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and MOCASSIN: 3D photoionisation and dust radiative transfer modelling of PNe will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-163998