Molecular transitions - PowerPoint PPT Presentation

ISM Lecture 12

ISM Lecture 12. Molecular Clouds I: Molecular spectroscopy, H 2. 12.1 Molecular structure. Ryb &amp; Lightman Chap. 11 Lectures H. Linnartz. All information about molecule is contained in Schrödinger equation ( R  positions of nuclei, x  positions of electrons): Hamilton operator:.

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The Emission Line Universe: Galactic Sources of Emission Lines

The Emission Line Universe: Galactic Sources of Emission Lines. Stephen S. Eikenberry University of Florida 22 November 2006. OUTLINE. Introduction Infrared Emission Lines Nebular Galactic Emission Line Sources Stellar Galactic Emission Line Sources Summary &amp; Future Prospects.

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