Published June 1986
| Version v1
Journal article
Low density ionized gas associated with M17, G333.3-0.4 and RCW74
Creators
- 1. Instituto Argentino de Radioastronomia, Buenos Aires
Description
We made observations in the H166 ∞ line and in the 1.4 GHz continuum at several positions in extended ionized gas associated with the H II regions M17, G333.3 - 0.4, and RCW 74, respectively. We derived electron temperatures and other physical parameters of these regions and compared them with those obtained by other authors from higher frequency radio recombination line observations. The results are compatible with a description of relatively extended H II regions, each consisting of a small compact region (Nsub(e)=100 to 1000cm-3) embedded in an extended ionizing gas envelope of lower density (Nsub(e)=1-10cm-3). Electron temperatures appear to vary with density, at least in M17. (authors)
Additional details
Publishing Information
- Journal Title
- Rev. Mex. Astron. Astrof.
- Journal Volume
- 13
- Journal Issue
- 1
- Series
- Rev. Mex. Astron. Astrof.
- Journal Page Range
- 15-25
- ISSN
- 0185-1101
- CODEN
- RMAAD
INIS
- Country of Publication
- Mexico
- Country of Input or Organization
- Mexico
- INIS RN
- 18025583
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- H2 REGIONS; INTERSTELLAR GRAINS; IONIZED GASES; LTE; NEBULAE; STAR ACCRETION
- Descriptors DEC
- COSMIC RADIO SOURCES; EQUILIBRIUM; FLUIDS; GASES; PARTICLES; STAR EVOLUTION