16O18O isotopomer collision rate (Marechal+ 1997)

Details 16O18O isotopomer collision rate (Marechal+ 1997) 16O18O isotopomer collision rate (Marechal+ 1997)

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ycat..33280617m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/328/617. Originally published in: 1997A&A...328..617M

Physics

Atomic Physics

Atomic Physics, Radio Lines

Scientific paper

In this paper, a chemical model of interstellar clouds including 18 and 13C isotopic reactions with a non-LTE calculations of 16O18O rotational population has been used to predict the intensity of the three 16O18O lines observable from the ground, namely 234, 298 and 402GHz. (3 data files).

Affiliated with

Also associated with

No associations

Rating

16O18O isotopomer collision rate (Marechal+ 1997) 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 16O18O isotopomer collision rate (Marechal+ 1997), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 16O18O isotopomer collision rate (Marechal+ 1997) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1481791