Far-infrared and submillimeter observations of stellar radiative and wind heating in S140 IRS

Details Far-infrared and submillimeter observations of stellar radiative and wind heating in S140 IRS Far-infrared and submillimeter observations of stellar radiative and wind heating in S140 IRS

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...271..625s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 271, Aug. 15, 1983, p. 625-631.

Astronomy and Astrophysics

Astronomy

35

Astronomical Maps, Infrared Astronomy, Interstellar Matter, Stellar Winds, Submillimeter Waves, Cosmic Dust, Gas Temperature, Plasma Interactions, Radiative Heat Transfer, Star Clusters, Temperature Distribution

Scientific paper

Far-infrared and submillimeter mapping of S140 IRS presents a picture of
heating of the dust in this condensation by the radiation and stellar
winds of a small star cluster. Comparison of dust and gas temperature
distributions implies good coupling between the gas and dust and nearly
equal dust and gas temperatures.

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