Far-infrared cooling lines in pre-MS sources

Details Far-infrared cooling lines in pre-MS sources Far-infrared cooling lines in pre-MS sources

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.427..575s&link_type=abstract

The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427., p. 575

Physics

11

Stars: Circumstellar Matter, Stars: Pre-Main Sequence, Infrared: Spectroscopy, Infrared: Molecular Lines

Scientific paper

We review the results of the observations in the 45-190 μm wavelength
range with the ISO Long Wavelength Spectrometer of a sample of Class 0,
Class I, Class II pre-Main Sequence objects. We briefly discuss the role
of [OI] and of molecular lines in the cooling of these sources.

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