Thermodynamic properties of the sources IRAS 05391-0217 and IRAS 06572-0742.

Details Thermodynamic properties of the sources IRAS 05391-0217 and IRAS 06572-0742. Thermodynamic properties of the sources IRAS 05391-0217 and IRAS 06572-0742.

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999acasn..40...44l&link_type=abstract

Acta Astron. Sin., Vol. 40, No. 1, p. 44 - 50

Other

Interstellar Clouds: Thermal Structure, Interstellar Clouds: Carbon Monoxide, Interstellar Clouds: Infrared Sources

Scientific paper

By analyzing the CO J = 1-0 spectra of IRAS 05391-0217 and IRAS 06572-0742 the authors calculated the gas kinetic temperature distributions of the two sources. With the IRAS and other infrared data, they fitted the dust thermal structures and investigated their thermal equilibria. In the case of Td < Tk in IRAS 05391-0217, they considered several possible heating mechanisms. The calculation shows that the photoelectric heating may be important. There is also high-velocity gas in the cloud discussed, so the shock heating can be another possible mechanism.

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