The electron temperatures of W 31 C and S 206

Details The electron temperatures of W 31 C and S 206 The electron temperatures of W 31 C and S 206

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....95..388c&link_type=abstract

Astronomy and Astrophysics, vol. 95, no. 2, Mar. 1981, p. 388-390. Research supported by the Consejo Nacional de Ciencia y Tecn

Astronomy and Astrophysics

Astrophysics

5

Electron Energy, H Alpha Line, Interstellar Gas, Radio Spectra, Abundance, Emission Spectra, Galactic Nuclei, H Ii Regions, Hydrogen Recombinations, Thermodynamic Equilibrium

Scientific paper

Radio recombination line observations are used to determine the electron temperatures of the H II regions W31C and S206. The data seem to confirm the conclusion of Mezger et al. (1979) that there is very little gradient in the electron temperature of H II regions located at galactocentric distances greater than 9 kpc. Most of the decrease in electron temperature occurs rather abruptly in the region inside 9 kpc.

Affiliated with

Also associated with

No associations

Rating

The electron temperatures of W 31 C and S 206 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 The electron temperatures of W 31 C and S 206, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The electron temperatures of W 31 C and S 206 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1785507