Published June 1986 | Version v1
Journal article

Low density ionized gas associated with M17, G333.3-0.4 and RCW74

  • 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