lecture7 - k(T) = A(T) exp(-E /kT) a H H H 2 Formation of...

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OMC: KL HOT CORES
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IRC10216 molecular maps
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Gaseous interstellar and circumstellar molecules  (149) N=2 N=3 N=4 N = 5 N = 6 N = 7 N = 8 N = 9 N = 10 2 AlCl CH 2 C 2 S NH 3 CH 4 CH 3 OH CH 3 NH 2 HCOOCH 3 (CH 3 ) 2 O (CH 3 ) 2 CO
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Diffuse Interstellar Bands
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Cosmic rays produce ions A + B C + D activation energy POTENTIAL ENERGY OF REACTION typical neutral reactions radical-radical reactions ion-molecule reactions
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Unformatted text preview: k(T) = A(T) exp(-E /kT) a H H H 2 Formation of Hydrogen dust particle FORMATION OF GASEOUS WATER H 2 + COSMIC RAYS H 2 + + e Elemental abundances: C,O,N = 10(-4); C<O Elemental abundances: C,O,N = 10(-4); C<O H 2 + + H 2 H 3 + + H H 3 + + O OH + + H 2 OH n + + H 2 OH n+1 + + H...
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This note was uploaded on 06/13/2011 for the course CHEMISTRY 740 taught by Professor Herbst during the Winter '08 term at Ohio State.

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lecture7 - k(T) = A(T) exp(-E /kT) a H H H 2 Formation of...

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