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Planetary Nebulae and Interstellar Medium
The Cold ISM
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  • Planetary Nebulae and Interstellar Medium
    • Einführung
    • Die Spektren der Gasnebel
    • Qualitative Interpretation der Nebelspektren
    • Photoionisationsgleichgewicht
    • Thermisches Gleichgewicht
    • Berechnung des emittierten Spektrums
    • Line Diagnostics
    • Häufigkeit chemischer Elemente
    • Planetarische Nebel
    • The Cold ISM
PDF of this chapter: ismchap10.pdf (5.0 MB)
The Milky Way
Milky Way: Overview, Milky Way: ISM
Molecules: History
Molecules: History
Molecular Spectroscopy
Molecular Hamiltonian, Electronic States, Vibrations, Rotational Spectra, Reality, Selection Rules
Molecules: Molecular Hydrogen
Molecular Hydrogen
Molecules: Carbon Monoxide
Carbon Monoxide, CO: Isotope Effects, Column from Lines, NGC 2024, From CO to H
Molecular Clouds
Cloud Properties, All Molecules
Molecule Formation
The Problem, The Solution, Hydrogen Molecule
Grains
Depletion of Elements, Extinction, Scattering Halos: IC 435, X-Ray Dust Scattering Halos, Dust Models, Dust Models: The IRAS Challenge, Extended Red Emission, UIBs, PAHs, Dust Formation
Star Formation
Star Formation, Initial Collapse, Formation of protostar, Formation of Disk and Wind, Unveiling of Protostar
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Jörn Wilms / wilms@astro.uni-tuebingen.de