Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.310..181r&link_type=abstract
Astrophysics and Space Science, Volume 310, Issue 3-4, pp. 181-188
Astronomy and Astrophysics
Astrophysics
1
Astrochemistry, Ism: Abundances, Ism: Clouds, Ism: Molecules, Stars: Formation
Scientific paper
We have observed emission from both ortho and para spin states of ketene (CH2CO) towards several deeply-embedded protostars. The low CH2CO fractional abundances (˜10-10) and the rotation temperatures (˜20 K) are consistent with emission from the cooler envelope. We compare our results with previous studies and discuss possible production pathways to interstellar ketene. We suggest that, if low observed excitation temperatures of CH2CO, CH3CHO and H2CO are indicative of their absence from the hot core region, then this may be due to the extensive hydrogenation of pre-existing grain mantles prior to evaporation into the inner envelope, leading to lower abundances of these compounds and to mantles rich in alcohols.
Butner Harold M.
Charnley Steven B.
Ehrenfreund Pascale
Huang Hui-Chun
Kuan Yi-Jehng
No associations
LandOfFree
Organic astrochemistry: observations of interstellar ketene 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 Organic astrochemistry: observations of interstellar ketene, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Organic astrochemistry: observations of interstellar ketene will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-958902