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New Laboratory and Theoretical Studies of Astrophysically Important Reactions of H 3 +

New Laboratory and Theoretical Studies of Astrophysically Important Reactions of H 3 +. Ben McCall. Dept. of Chemistry. Dept. of Astronomy. Outline. Background Importance of H 3 + Interstellar Clouds H 3 + in Diffuse Clouds Abundance: H 3 + + e - ? H + H + H

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Analytics for Cold Hydrogen Isotopologues at the Tritium Laboratory Karlsruhe

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The (3, 3) metastable rotational level of H 3 +

The (3, 3) metastable rotational level of H 3 +. Takeshi Oka. Department of Chemistry and Department of Astronomy and Astrophysics The Enrico Fermi Institute, The University of Chicago. New Horizon of Astrochemistry and Laboratory Spectroscopy March 16, 9 am, 2006.

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Chapter 12: Reactions of Arenes: Electrophilic Aromatic Substitution 12.1: Representative Electrophilic Aromatic Substitution Reactions of Benzene. E= -Cl, -Br, -I (halogenation) -NO 2 (nitration) -SO 3 H (sulfonation) -R (alkylation) (acylation).

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Aromatic Reactions

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CASSIS - Java programs for the analysis of astrophysical spectra

2 ANALYSE SPECTRA SPECIES BY SPECIES. Predict spectra over wide frequency ranges at different temperatures. 1 MAKE PREDICTIONS. Spectroscopic databases. Collisional databases. Data from telescope. First-level data treatment. MODEL. Optimize parameters. Synthetic spectrum.

108 views • 1 slides