Solid CO in the Taurus dark clouds

Details Solid CO in the Taurus dark clouds Solid CO in the Taurus dark clouds

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.216p..45w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 216, Sept. 15, 1985, p. 45P-50P.

Astronomy and Astrophysics

Astronomy

61

Carbon Monoxide, Interstellar Matter, Millimeter Waves, Molecular Clouds, Solidified Gases, Taurus Constellation, Optical Thickness, Solid State, Vapor Pressure

Scientific paper

The infrared vibrational feature of solid state CO at 4.67 μm wavelength is detected towards five sources in or behind the dark cloud complex in Taurus. A comparison with millimetre-wave data suggests that a significant fraction (up to 40 per cent) of the CO may be depleted on to grains. The adjacent CN feature at 4.62 μm observed in W33A by Lacy et al. is absent from the authors' spectra, suggesting that the grain mantles in Taurus are unannealed.

Affiliated with

Also associated with

No associations

Rating

Solid CO in the Taurus dark clouds 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 Solid CO in the Taurus dark clouds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solid CO in the Taurus dark clouds will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-801946