CH+ Production in J-type Shocks

Details CH+ Production in J-type Shocks CH+ Production in J-type Shocks

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...189.1708p&link_type=abstract

American Astronomical Society, 189th AAS Meeting, #17.08; Bulletin of the American Astronomical Society, Vol. 28, p.1296

Astronomy and Astrophysics

Astronomy

Scientific paper

Numerical models of the chemistry of multi-fluid MHD shocks in diffuse molecular clouds have been calculated; 36 species were studied obtaining column densities and line profiles; special attention was given to CH(+) , CH and OH production. Particular attention has been given to J-type shocks, which have thus far been unexplored, for densities in the range of 15 cm(-3) <= n_H <= 50 cm(-3) with molecular hydrogen abundance of 0.2 <= H/H_2 <= 5. Excitation of H_2 in the shock was studied with predicted column densities of rotationally excited levels. Implications for the production of interstellar CH(+) will be discussed.

Affiliated with

Also associated with

No associations

Rating

CH+ Production in J-type Shocks 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 CH+ Production in J-type Shocks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CH+ Production in J-type Shocks will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-815186