Monte Carlo Radiative Transfer Calculations with Clumpy Cloud Models

Details Monte Carlo Radiative Transfer Calculations with Clumpy Cloud Models Monte Carlo Radiative Transfer Calculations with Clumpy Cloud Models

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pcim.conf..220j&link_type=abstract

The Physics and Chemistry of the Interstellar Medium, Proceedings of the 3rd Cologne-Zermatt Symposium, held in Zermatt, Septemb

Physics

Scientific paper

We describe a Monte Carlo code that is used to simulate the radiative transfer in clumpy medium. The program has been used to study the molecular line emission from interstellar clouds and individual cloud cores. The same methods can be applied to continuum radiation. This way the effects that a clumpy density structure will have on infrared dust emission can be studied. Some results of these studies are shown.

Affiliated with

Also associated with

No associations

Rating

Monte Carlo Radiative Transfer Calculations with Clumpy Cloud Models 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 Monte Carlo Radiative Transfer Calculations with Clumpy Cloud Models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Monte Carlo Radiative Transfer Calculations with Clumpy Cloud Models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1016747