Published February 1989 | Version v1
Journal article

Collisional rate coefficients of C3H2 and the determination of physical conditions in molecular clouds

  • 1. NASA, Goddard Institute for Space Studies, New York, NY (USA)
  • 2. National Research Council of Canada, Herzberg Institute of Astrophysics, Ottawa

Description

Collisional excitation rates for C3H2, calculated using the coupled states approximation at temperatures of 10-30 K, are presented. C3H2 produces a number of spectral line pairs whose members are close together in frequency but arise from levels with different excitation energies. The rates are used in statistical equilibrium calculations to illustrate the excitation properties and density-dependent behavior of various C3H2 line ratios. 17 references

Additional details

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
337
Series
Astrophys. J.
Journal Page Range
306-317
ISSN
0004-637X
CODEN
ASJOA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
20062649
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CHEMICAL COMPOSITION; COSMIC GASES; EXCITATION; HYDROCARBONS; INTERSTELLAR SPACE; LOW TEMPERATURE; MOLECULE COLLISIONS; SPECTRA; VERY LOW TEMPERATURE
Descriptors DEC
COLLISIONS; ENERGY-LEVEL TRANSITIONS; FLUIDS; GASES; ORGANIC COMPOUNDS; SPACE