Bell, K. L.; Williams, D. A. The radiation field and the molecular hydrogen photodissociation rate within spherically symmetric inhomogeneous clouds. (English) Zbl 0508.76075 Mon. Not. R. Astron. Soc. 202, 407-416 (1983). Page: −5 −4 −3 −2 −1 ±0 +1 +2 +3 +4 +5 Show Scanned Page MSC: 76E20 Stability and instability of geophysical and astrophysical flows 85A25 Radiative transfer in astronomy and astrophysics 76X05 Ionized gas flow in electromagnetic fields; plasmic flow Keywords:radiation field; H2 photodissociation rate; spherically symmetric inhomogeneous clouds; non-scattering grains PDFBibTeX XMLCite \textit{K. L. Bell} and \textit{D. A. Williams}, Mon. Not. R. Astron. Soc. 202, 407--416 (1983; Zbl 0508.76075) Full Text: DOI