"Complete" models of young stellar objects: the spectral energy distributions of embedded YSO's with and without disks.

Details "Complete" models of young stellar objects: the spectral energy distributions of embedded YSO's with and without disks. "Complete" models of young stellar objects: the spectral energy distributions of embedded YSO's with and without disks.

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992dudi.work..105b&link_type=abstract

"Dusty Discs, Proceedings of the 9th RAL Workshop on Astronomy and Astrophysics. Edited by P.M. Gondhalekar.

Astronomy and Astrophysics

Astrophysics

Scientific paper

Current star formation theories contain three components: the central source, a disk, and the collapsing envelope. In order to test star formation theories, it is necessary to study what are the observable consequences of each of the different components. To date, most radiative transfer models have focused on a central source and either an envelope or a disk. The author discusses a technique that allows him to combine all three elements (star, disk, and envelope) into a single radiative transfer model. The technique, which he refers to as the "spherical disk" approximation, allows him to assess the possible contributions of disks around embedded young stars to the overall spectral energy distribution. The author presents models where disks have been added to the central source function of L1551-IRS 5, a source he has previously modeled with star and envelope alone. He discusses the implications for both the overall spectral energy distribution and the millimeter interferometer data. In addition, the author discusses what effects an envelope can have on the disk and how this might change conclusions about the overall disk properties. Finally, the author points out the possible effect warm envelopes can have on T Tauri systems.

Affiliated with

Also associated with

No associations

Rating

"Complete" models of young stellar objects: the spectral energy distributions of embedded YSO's with and without disks. 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 "Complete" models of young stellar objects: the spectral energy distributions of embedded YSO's with and without disks., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and "Complete" models of young stellar objects: the spectral energy distributions of embedded YSO's with and without disks. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1114267