Chemical and thermal equilibrium in dark clouds. II - Importance of grain surface reactions for molecular formation

Details Chemical and thermal equilibrium in dark clouds. II - Importance of grain surface reactions for molecular formation Chemical and thermal equilibrium in dark clouds. II - Importance of grain surface reactions for molecular formation

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....73..174v&link_type=abstract

Astronomy and Astrophysics, vol. 73, no. 1-2, Mar. 1979, p. 174-182.

Astronomy and Astrophysics

Astrophysics

16

Chemical Equilibrium, Hydrogen Clouds, Interstellar Chemistry, Surface Reactions, Thermodynamic Equilibrium, Cooling, Gas Heating, Graphs (Charts), Interstellar Gas, Radiative Transfer, Ultraviolet Radiation

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1979A&A....73..174V

Affiliated with

Also associated with

No associations

Rating

Chemical and thermal equilibrium in dark clouds. II - Importance of grain surface reactions for molecular formation 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 Chemical and thermal equilibrium in dark clouds. II - Importance of grain surface reactions for molecular formation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chemical and thermal equilibrium in dark clouds. II - Importance of grain surface reactions for molecular formation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1648804