Modeling the Ultracompact HII Regions and Comparison with ISO Mid-Infrared Spectroscopy

Details Modeling the Ultracompact HII Regions and Comparison with ISO Mid-Infrared Spectroscopy Modeling the Ultracompact HII Regions and Comparison with ISO Mid-Infrared Spectroscopy

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..267..441w&link_type=abstract

Hot Star Workshop III: The Earliest Stages of Massive Star Birth. ASP Conference Proceedings, Vol. 267. Edited by Paul A. Crowth

Astronomy and Astrophysics

Astronomy

Scientific paper

Photo-ionization and dust shell models of ultracompact HII region are presented. The model predictions are directly compared with observed properties (e.g., line intensities, continuum emission from dust) obtained by ISO mid-infrared spectroscopy, and the characteristics of the embedded ionizing star(s) and the dust distribution are reported for the observed HII regions.

Affiliated with

Also associated with

No associations

Rating

Modeling the Ultracompact HII Regions and Comparison with ISO Mid-Infrared Spectroscopy 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 Modeling the Ultracompact HII Regions and Comparison with ISO Mid-Infrared Spectroscopy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling the Ultracompact HII Regions and Comparison with ISO Mid-Infrared Spectroscopy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1661683