Physical conditions in the H II region S106 according to observations of radio recombination lines of hydrogen and helium

Details Physical conditions in the H II region S106 according to observations of radio recombination lines of hydrogen and helium Physical conditions in the H II region S106 according to observations of radio recombination lines of hydrogen and helium

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..209e&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, March 1988, p. 209-215. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Electron Recombination, H Ii Regions, H Lines, Helium, Nebulae, Radio Spectra, Astronomical Models, Electron Density Profiles

Scientific paper

Observations of the S 106 nebula in the hydrogen and helium radio
recombination lines (H56α, H66α and He66α) at
frequencies 36.5 and 22.4 GHz have been made at the Pushchino Radio
Astronomy Station. A core-halo model is proposed.

Affiliated with

Also associated with

No associations

Rating

Physical conditions in the H II region S106 according to observations of radio recombination lines of hydrogen and helium 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 Physical conditions in the H II region S106 according to observations of radio recombination lines of hydrogen and helium, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Physical conditions in the H II region S106 according to observations of radio recombination lines of hydrogen and helium will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1692223