Far-Infrared Investigation of Class 0 Sources: Line Cooling

Details Far-Infrared Investigation of Class 0 Sources: Line Cooling Far-Infrared Investigation of Class 0 Sources: Line Cooling

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001apj...555...40g&link_type=abstract

The Astrophysical Journal, Volume 555, Issue 1, pp. 40-57.

Astronomy and Astrophysics

Astronomy

80

Infrared: Ism, Ism: Jets And Outflows, Ism: Molecules, Stars: Formation, Stars: Mass Loss

Scientific paper

We have investigated with the Long Wavelength Spectrometer (LWS) of the Infrared Space Observatory (ISO) the far-infrared spectra (43-197 μm) of a sample of 17 class 0 sources and their associated outflows. In addition to [O I] 63 μm, the pure rotational lines of abundant molecules such as CO, H2O, and OH are frequently observed in these sources, at variance with more evolved young stellar objects. We found, in agreement with previous studies conducted on individual sources, that the molecular line excitation arises from small regions, with typical sizes of 10-9 sr, of warm (200

Affiliated with

Also associated with

No associations

Rating

Far-Infrared Investigation of Class 0 Sources: Line Cooling does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Far-Infrared Investigation of Class 0 Sources: Line Cooling, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Far-Infrared Investigation of Class 0 Sources: Line Cooling will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1773948