Construction of theoretical spectra for compact H II regions

Details Construction of theoretical spectra for compact H II regions Construction of theoretical spectra for compact H II regions

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pazh....3..359t&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 3, Aug. 1977, p. 359-362. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Emission Spectra, H Ii Regions, Spectrum Analysis, Stellar Evolution, Cosmic Dust, Gas Density, Gas Temperature, Infrared Radiation

Scientific paper

Theoretical emission spectra in the frequency range from 10 to the 7th power to 10 to the 15.5 power Hz are constructed on the basis of simplified evolutionary models of compact H II regions. The computed spectrum is a combination of thermal radiation from the ionized hydrogen zone, infrared radiation from a gas-dust shell, and stellar radiation penetrating the shell during late stages in the development of a cocoon. Comparison shows that these spectra are in qualitative agreement with the observed spectra of the compact H II region W3 (A).

Affiliated with

Also associated with

No associations

Rating

Construction of theoretical spectra for compact H II regions 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 Construction of theoretical spectra for compact H II regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Construction of theoretical spectra for compact H II regions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1881305