Static Chemistry in Disks or Clouds

Details Static Chemistry in Disks or Clouds Static Chemistry in Disks or Clouds

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006asd..soft...26s&link_type=abstract

Astrophysics Software Database, CAU Kiel, Germany (http://www1.astrophysik.uni-kiel.de/asd/).

Astronomy and Astrophysics

Astrophysics

Fortran

Scientific paper

This FORTRAN77 code can be used to model static, time-dependent chemistry in ISM and circumstellar disks. Current version is based on the OSU'06 gas-grain astrochemical network with all updates to the reaction rates, and includes surface chemistry from Hasegawa & Herbst (1993) and Hasegawa, Herbst, and Leung (1992). Surface chemistry can be modeled either with the standard rate equation approach or modified rate equation approach (useful in disks). Gas-grain interactions include sticking of neutral molecules to grains, dissociative recombination of ions on grains as well as thermal, UV, X-ray, and CRP-induced desorption of frozen species. An advanced X-ray chemistry and 3 grain sizes with power-law size distribution are also included. An deuterium extension to this chemical model is available.

Affiliated with

Also associated with

No associations

Rating

Static Chemistry in Disks or 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 Static Chemistry in Disks or Clouds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Static Chemistry in Disks or Clouds will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1311477