Modeling of diffuse interstellar clouds - The case of Gamma Arae

Details Modeling of diffuse interstellar clouds - The case of Gamma Arae Modeling of diffuse interstellar clouds - The case of Gamma Arae

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....89..113f&link_type=abstract

Astronomy and Astrophysics, vol. 89, no. 1-2, Sept. 1980, p. 113-117.

Astronomy and Astrophysics

Astrophysics

9

Astrophysics, Interstellar Chemistry, Interstellar Gas, Cosmic Dust, Density Distribution, Hydrogen, Neutral Gases

Scientific paper

Observations of the interstellar cloud toward Gamma Arae (Morton and Hu, 1975) are analyzed with an improved version of the isobaric, steady-state model of Glassgold and Langer (1974). Good agreement is obtained using parameters which are close to those which represent the average properties of many diffuse interstellar clouds. The successful correlation of the data for H, H2, C II, C I, OI, CO, and OH supports current concepts on interstellar thermodynamics and chemistry.

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