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OMC: KL

OMC: KL. HOT CORES. IRC10216 molecular maps. Gaseous interstellar and circumstellar molecules (149). Diffuse Interstellar Bands. Cosmic rays produce ions. FORMATION OF GASEOUS WATER. H 2 + COSMIC RAYS  H 2 + + e. Elemental abundances: C,O,N = 10(-4); C<O.

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OMC: KL

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  1. OMC: KL HOT CORES

  2. IRC10216 molecular maps

  3. Gaseous interstellar and circumstellar molecules (149)

  4. Diffuse Interstellar Bands

  5. Cosmic rays produce ions

  6. FORMATION OF GASEOUS WATER H2 + COSMIC RAYS  H2+ + e Elemental abundances: C,O,N = 10(-4); C<O Elemental abundances: C,O,N = 10(-4); C<O H2+ + H2 H3+ + H H3+ + O  OH+ + H2 OHn+ + H2  OHn+1+ + H H3O+ + e  H2O + H; OH + 2H, etc

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