2022 — The KOSMA-τ PDR model. I. Recent updates to the numerical model of photo-dissociated regions
Röllig, M and Ossenkopf-Okada, V.), 2022, Astronomy & Astrophysics, Volume 664, id.A67, 43 pp.
Keywords: photon dominated regions, astrochemistry, physics of the interstellar medium, numerical simulation
KOSMA-tau is a numerical code to compute the physical and chemical structure of a spherical molecular cloud, a so called photo-dissociation region (PDR). This code has been developed from an earlier PDR code, written by A. Sternberg from Tel Aviv University in Israel (Sternberg & Dalgarno 1989; Sternberg & Dalgarno 1995). His original code uses a plane-parallel geometry and was updated to employ spherical geometry (Gierens, Stutzki and Winnewisser 1992; Köster et al. 1994; Störzer, Stutzki and Sternberg 1996; Zielinsky, Stutzki & Störzer 2000).
The different ‘blocks’ in the mentioned scheme depend on each other which makes an iterative solution necessary. The result is a the chemical and physical structure of the model cloud as a function of radius.
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Röllig, M and Ossenkopf-Okada, V.), 2022, Astronomy & Astrophysics, Volume 664, id.A67, 43 pp.
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