Synonyms
Definition
A photodissociation region (PDR) is an interstellar gas phase in which far-ultraviolet (FUV; 6 eV < hν < 13.6 eV, where eV is the energy of the radiation in electron volts) radiation plays a role in the heating and/or chemistry (Tielens and Hollenbach 1985a). These regions include the diffuse atomic interstellar medium, and the surfaces of interstellar molecular clouds exposed to the interstellar radiation field and to intense radiation from nearby OB stars. Note that in the following article we use the standard astronomical notation of square brackets (e.g., [CII]) indicating “forbidden” transitions, that is, transitions from a metastable state. Likewise, the ionization state of an atom is indicated by a Roman numeral, so that I indicates the neutral atom, II is once ionized, and so on (e.g., HII for ionized hydrogen).
Overview
The FUV range of energies is responsible for dissociating molecules and dominates the heating process in...
References and Further Reading
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Wolfire, M.G., Kaufman, M.J. (2014). Photodissociation Region. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1197-8
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DOI: https://doi.org/10.1007/978-3-642-27833-4_1197-8
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