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Titlebook: Astrophysics of the Diffuse Universe; Michael A. Dopita,Ralph S. Sutherland Textbook 2003 Springer-Verlag Berlin Heidelberg 2003 Astrochem

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發(fā)表于 2025-3-25 07:16:54 | 只看該作者
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Platform Game: Physics and Data Management,ming from a photoionizing source, be it a star, a nucleus of an active galaxy, or whatever. Such photoionization-dominated plasmas are very commonly observed in galaxies and historically, were one of the first to be studied in detail, thanks to their bright and prominent emission line spectra at opt
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Controlling a Player Character,l bulge of faint Galactic stars is crossed by dark lanes, filaments, and clouds of dense dusty gas made visible in projection. Because the dust grains are very small, typically less than a micron in diameter, their absorption characteristics are very wavelength dependent, and blue or ultraviolet pho
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發(fā)表于 2025-3-26 05:12:20 | 只看該作者
Platform Game: Physics and Data Management, crisscrossed by violent shocks and pervaded by intense UV and X-ray radiation fields, which can easily tear apart delicate molecular bonds. Even the composition of the interstellar medium presents a problem to the formation of complex molecules, since the gas is mostly hydrogen and helium. Reactive
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https://doi.org/10.1007/978-1-4302-4717-3which form new stars, new winds, and new supernovae in their turn, it is roiled, churned, and compressed to produce a ramified skein of cooler atomic or molecular gas embedded in hotter ionized phases. The spatial structure of these various thermal phases is driven by the interstellar gas seeking to
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