H II regions and CO clouds - The blister model

Details H II regions and CO clouds - The blister model H II regions and CO clouds - The blister model

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....70..769i&link_type=abstract

Astronomy and Astrophysics, vol. 70, no. 6, Dec. 1978, p. 769-775.

Astronomy and Astrophysics

Astronomy

154

Astronomical Models, Carbon Monoxide, H Ii Regions, Interstellar Matter, Radio Astronomy, Astronomical Maps, Gas Ionization, Hydrogen Ions, Radial Velocity, Statistical Analysis, Stellar Evolution

Scientific paper

A comparison of H II region and CO cloud observations shows that the majority of H II regions are located at the edges of molecular clouds, and have structure suggestive of ionization fronts surrounded by less dense envelopes. The bulk of the ionized material streams away from the associated molecular cloud. The general applicability of this blister model has important consequences for models of both H II region evolution and star formation.

Affiliated with

Also associated with

No associations

Rating

H II regions and CO clouds - The blister model 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 H II regions and CO clouds - The blister model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and H II regions and CO clouds - The blister model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-885629