Time-dependent radiative cooling of a hot, optically thin interstellar gas

Details Time-dependent radiative cooling of a hot, optically thin interstellar gas Time-dependent radiative cooling of a hot, optically thin interstellar gas

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993astl...19...11k&link_type=abstract

Astronomy Letters, Vol. 19, p. 11-13; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 19, no. 1, p. 27-33. In Russian.

Astronomy and Astrophysics

Astronomy

7

Interstellar Gas, Luminescence, Radiant Cooling, Energy Dissipation, High Temperature Gases

Scientific paper

Calculations are presented for the radiative cooling of a hot low-density interstellar gas. It is shown that a strong dependence of the radiative energy loss on the abundance of the chemical elements of the gas exists in the range 10 exp 4.5-10 exp 6.5 K. The radiative energy loss functions differ insignificantly in the time-dependent cases, but isobaric cooling takes less time than the isochoric one.

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