Photodissociation Fronts

Bruce T. Draine, Dept. of Astrophysical Sciences, Princeton University

Recent Papers

• Weingartner, J.C., & Draine, B.T. 2001, "Photoelectric Emission from Interstellar Dust: Grain Charging and Gas Heating", Astrophys. J. Suppl., 135, 000-000 (2001 July) (astro-ph/9907251)
• Weingartner, J.C., & Draine, B.T. 2001, "Forces on Dust Grains Exposed to Anisotropic Radiation Fields", Astrophys, J., 553, 000-000 (2001 May 20) (astro-ph/0010117)
• Bertoldi, F., Draine, B.T., Rosenthal, D., Timmermann, R., Ramsay Howat, S.K., Geballe, T., Feuchtgruber, H., and Drapatz, S. 2000 "Excitation of H2 and HD in shocks and PDRs", in IAU Symposium 197: Astrochemistry, ed. Y.C. Minh and E.F. van Dishoeck (San Francisco: Astr. Soc. Pacific), p. 191-201 (astro-ph/0009384)
• Draine, B.T., and Bertoldi, F. 2000, "Theoretical Models of Photodissociation Fronts", in H2 in Space, ed. F. Combes and G. Pineau des Forets (Cambridge: Cambridge Univ. Press), 131-138 (astro-ph/0008149)
• Bertoldi, F., Draine, B.T., Rosenthal, D., Timmermann, R., Ramsay Howat, S.K., Geballe, T., Feuchtgruber, H., and Drapatz, S. 2000 "Excitation of H2 and HD in shocks and PDRs", in IAU Symposium 197: Astrochemistry, ed. Y.C. Minh and E.F. van Dishoeck (San Francisco: Astr. Soc. Pacific), p. 191-201 (astro-ph/0009384)
• Draine, B.T. 2000, "Gamma Ray Bursts in Molecular Clouds: H2 Absorption and Fluorescence", Astrophys. J., 532, 273-280 (astro-ph/9907232)
• Draine, B.T., & Bertoldi, F. 1999, "Heating the Gas in Photodissociation Fronts'', in The Universe As Seen By ISO, ed. P. Cox & M.F. Kessler, (Noordwijk: ESA), 553-559 (astro-ph/9902379)
• Vicini, B., Natta, A., Marconi, A., Testi, L., Hollenbach, D., & Draine, B.T. 1999, "A Near-Infrared Study of the Planetary Nebula NGC 2346", Astron. Astrophys., 342, 823-830.
• Bertoldi, F., Draine, B.T., Drapatz, S. Rosenthal, D., Timmerman, R., Wright, C.M. 1999, "ISO looks at shocks and photodissociation regions", in The Physics and Chemistry of the Interstellar Medium, Proceedings of the 3rd Cologne-Zermatt Symposium, ed. V. Ossenkopf, J. Stutzki, & G. Winnewisser (GCA-Verlag Herdecke), 120 <
• Timmermann, R., Bertoldi, F., Wright, C.M., Drapatz, S., Draine, B.T., Haser, L., & Sternberg, A. 1996, "H_2 infrared line emission from S140: a warm PDR", Astr. Ap., 315, L281.
• Draine, B.T., & Bertoldi, F. 1996, "Structure of Stationary Photodissociation Fronts", Astrophys. J., 468, 269 ( POPe-634.ps.gz).
• Bertoldi, F., & Draine, B.T. 1996, "Non-Equilibrium Photodissociation Regions: I. Ionization-Dissociation Fronts", Astrophys. J., 458, 222.

Catalog of PDR Models

• am3d (n=10^2,chi=1,diff.dust,T_0=300,cos(theta)=1) file= spdf.irs.am3d.Z
• am3o (n=10^2,chi=1,orion dust,T_0=300,cos(theta)=1) file= spdf.irs.am3o.Z
• aw3d (n=10^2,chi=1,diff.dust,T_0=500,cos(theta)=1) file= spdf.irs.aw3d.Z
• aw3o (n=10^2,chi=1,orion dust,T_0=500,cos(theta)=1) file= spdf.irs.aw3o.Z
• bw3d (n=10^2,chi=10,diff.dust,T_0=500,cos(theta)=1) file= spdf.irs.bw3d.Z
• bw3o (n=10^2,chi=10,orion dust,T_0=500,cos(theta)=1) file= spdf.irs.bw3o.Z
• bh3d (n=10^2,chi=10,diff.dust,T_0=1000,cos(theta)=1) file= spdf.irs.bh3d.Z
• bh3o (n=10^2,chi=1,orion dust,T_0=1000,cos(theta)=1) file= spdf.irs.bh3o.Z
• Bm3o (n=10^3,chi=10,orion dust,T_0=300,cos(theta)=1) file= spdf.irs.Bm3o.Z
• Bw3o (n=10^3,chi=10,orion dust,T_0=500,cos(theta)=1) file= spdf.irs.Bw3o.Z
• Cw3o (n=10^3,chi=10^2,orion dust,T_0=500,cos(theta)=1) file= spdf.irs.Cw3o.Z
• Ch3o (n=10^3,chi=10^2,orion dust,T_0=1000,cos(theta)=1) file= spdf.irs.Ch3o.Z
• Gm3o (n=10^4,chi=10^2,orion dust,T_0=300,cos(theta)=1) file= spdf.irs.Gm3o.Z
• Gw3o (n=10^4,chi=10^2,orion dust,T_0=500,cos(theta)=1) file= spdf.irs.Gw3o.Z
• Hw3o (n=10^4,chi=10^3,orion dust,T_0=500,cos(theta)=1) file= spdf.irs.Hw3o.Z
• Hh3o (n=10^4,chi=10^3,orion dust,T_0=1000,cos(theta)=1) file= spdf.irs.Hh3o.Z
• Lm3o (n=10^5,chi=10^3,orion dust,T_0=300,cos(theta)=1) file= spdf.irs.Lm3o.Z
• Lw3o (n=10^5,chi=10^3,orion dust,T_0=500,cos(theta)=1) file= spdf.irs.Lw3o.Z
• Mw3o (n=10^5,chi=10^4,orion dust,T_0=500,cos(theta)=1) file= spdf.irs.Mw3o.Z
• Mh3o (n=10^5,chi=10^4,orion dust,T_0=1000,cos(theta)=1) file= spdf.irs.Mh3o.Z
• Qm3o (n=10^6,chi=10^4,orion dust,T_0=300,cos(theta)=1) file= spdf.irs.Qm3o.Z
• Qw3o (n=10^6,chi=10^4,orion dust,T_0=500,cos(theta)=1) file= spdf.irs.Qw3o.Z
• Rw3o (n=10^6,chi=10^5,orion dust,T_0=500,cos(theta)=1) file= spdf.irs.Rw3o.Z
• Rh3o (n=10^6,chi=10^5,orion dust,T_0=1000,cos(theta)=1) file= spdf.irs.Rh3o.Z
• n2023a (n=10^5,chi=5000,orion dust,T_0=500,cos(theta)=0.2) file= spdf.irs.n2023a.Z
• n2023b (n=10^5,chi=5000,orion dust,T_0=900,cos(theta)=0.2) file= spdf.irs.n2023b.Z

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