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From Molecules to Grains

Published online by Cambridge University Press:  12 April 2016

Erwin Sedlmayr
Erwin Sedlmayr*
Affiliation:
Institut für Astronomie und Astrophysik, Technische Universität Berlin, Hardenbergstr. 36, D-10623 Berlin, Germany

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Cosmic dust is an ubiquiteous component of the interstellar medium, the presence of which has severe bearings both upon the observations and upon the physical description and realistic modelling of astronomical objects. In most dusty objects, the grain component is intimately interwoven with the gas component and the radiation field, and, hence strongly affects the thermodynamical, the hydrodynamical and the chemical structure of the object. Therefore any consistent description of the astrophysical dust complex has to rely upon a treatment where these aspects are properly taken into account. In general this complex comprises the following problems:

  1. – Formation of small stable molecular clusters out of the gaseous phase

  2. – Growth of these clusters to macroscopic specimens (primary condensates: grains, plates, etc.)

  3. – Destruction of grains (e.g. thermal evaporation, sputtering, shattering), and

  4. – Physical and chemical processing of already existing grains (e.g. coagulation, chemical and thermal transformation, etc....).

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 146: Molecules in the Stellar Environment , 1994 , pp. 163 - 185
Copyright
Copyright © Springer-Verlag 1994

References

Allamandola, L.J., Tielens, A.G.G.M., Barker, J.R., 1987, In: Mortili, G.E., Scholer, M. (eds.), Physical Processes in Interstellar Clouds, Proc. NATO Advanced Study Institute, D. Reidel Publ. Comp., Dordrecht, p.365 Google Scholar
Augustin, K., 1990, Diplomarbeit, Technische Universität, Berlin Google Scholar
Beck, H.K.B., Gail, H.-P., Henkel, R., Sedlmayr, E., 1992, Astron. Astrophys,, 265, 626 Google Scholar
Castleman, A.W., 1979, Astrophys. Space Sei., 65, 337 CrossRefGoogle Scholar
Cherchneff, I., Barker, J.R., 1992, Astrophys. J., 394, 703 CrossRefGoogle Scholar
Cherchneff, L., Barker, J.R., Tielens, A.G.G.M., 1991, Astrophys. J., 377, 541 CrossRefGoogle Scholar
Cherchneff, I., Barker, J.R., Tielens, A.G.G.M., 1992, Astrophys. J., 401, 269 CrossRefGoogle Scholar
Dominik, C., Gail, H.-P., Sedlmayr, E., 1989, Astron. Astrophys., 223, 227 Google Scholar
Dominik, C., Gail, H.-P., Sedlmayr, E., Winters, J.M., 1990, Astron. Astrophys., 240, 365 Google Scholar
Dominik, C., Sedlmayr, E., Gail, H.-P., 1993, Astron. Astrophys., in pressGoogle Scholar
Donn, B., Hecht, J., Khanna, R., Nuth, J.A., Stranz, D., Anderson, A.D., 1981, Surface Sci., 106, 576 CrossRefGoogle Scholar
Draine, B.T., 1979, Astrophys. Space Sci. 65, 313 CrossRefGoogle Scholar
Draine, B.T., Salpeter, E.E., 1977, J. Chem. Phys., 67, 2230 CrossRefGoogle Scholar
Feder, D., Rüssel, K.C., Lothe, B., Pound, G.M., 1966, Advan. in Phys., 15, 111 CrossRefGoogle Scholar
Fleischer, A.J., Gauger, A., Sedlmayr, E., 1992, Astron. Astrophys., 266, 321 Google Scholar
Frenklach, M., Feigelson, E., 1989, Astrophys. J., 341, 372 CrossRefGoogle Scholar
Gail, H.-P., Sedlmayr, E., 1975, Astron. Astrophys., 41, 359 Google Scholar
Gail, H.-P., Sedlmayr, E., 1984, Astron. Astrophys., 132, 163 Google Scholar
Gail, H.-P., Sedlmayr, E., 1986, Astron. Astrophys., 166, 225 Google Scholar
Gail, H.-P., Sedlmayr, E., 1987, In: Morfill, G.E., Scholer, M. (eds.), Physical Processes in Interstellar Clouds, Proc. NATO Advanced Study Institute, D. Reidel Publ. Comp., Dordrecht, p.275 Google Scholar
Gail, H.-P., Sedlmayr, E., 1988, Astron. Astrophys., 206, 153 Google Scholar
Gauger, A., Gail, H.-P., Sedlmayr, E., 1990, Astron. Astrophys., 235, 345 Google Scholar
Gehrz, R.D., 1989, In: Allamandola, L.J. & Tielens, A.G.G.M. (eds.), Interstellar Dust, Proc. IAUSymp. No. 135, D.Reidel Publ Comp., Dordrecht, p.445 CrossRefGoogle Scholar
Goeres, A., 1993, In: Klare, G. (ed.), Reviews in Modern Astronomy, 6, Springer, p.165 Google Scholar
Goeres, A., Sedlmayr, E., 1991, Chem. Phys. Letters, 184, 310 CrossRefGoogle Scholar
Goeres, A., Sedlmayr, E., 1992, Astron. Astrophys., 265, 216 Google Scholar
Goeres, A., Henkel, R., Sedlmayr, E., Gail, H.-P., 1988, In: Klare, G. (ed.), Reviews in Modern Astronomy, 1, Springer, p.231 Google Scholar
Greenberg, J.M., 1989, In: Allamandola, L.J. & Tielens, A.G.G.M. (eds.), Interstellar Dust, Proc. IAU Symp. No. 135, D.Reidel Publ Comp., Dordrecht, p.345 CrossRefGoogle Scholar
Jenkins, E.B., 1989, In: Allamandola, L.J. & Tielens, A.G.G.M. (eds.), Interstellar Dust, Proc. IAUSymp. No. 135, D. Reidel Publ Comp., Dordrecht, p.23 CrossRefGoogle Scholar
Jura, M., 1986, Astrophys. I., 303, 327 CrossRefGoogle Scholar
Keller, R., 1987, In: Léger, A., d'Hendecourt, L., Boceara, N. (eds.), PolycycUc Aromatic Hydrocarbons and Astrophysics, Proc. NATO Advanced Study Institute, D. Reidel Publ. Comp., Dordrecht, p.387 Google Scholar
Keller, R., Sedlmayr, E., 1983, Mitt. Astron. Ges., 60, 312 Google Scholar
Knapp, G.R., 1985, Astrophys. J., 293, 273 CrossRefGoogle Scholar
Köhler, M., 1993, Dissertation, Technische Universität, Berlin, in prep.Google Scholar
Kozasa, T., Hasegawa, H., 1987, Prog. Theor. Phys., 77, 1402 CrossRefGoogle Scholar
Kozasa, T., Hasegawa, H., Nomoto, K., 1989a, Astrophys. J., 344, 325 CrossRefGoogle Scholar
Kozasa, T., Hasegawa, H., Nomoto, K., 1989b, Astrophys. J., 346, L81 CrossRefGoogle Scholar
Krätschmer, W., Fostiropoulos, K., Huffman, D.R., 1990, Chem. Phys. Lett. 170, 167 CrossRefGoogle Scholar
Krüger, M., 1992, Diplomarbeit, Technische Universität, Berlin Google Scholar
Lafon, J.P.J., Berruyer, N., 1991, Astron. Astrophys. Rev., 2, 291 CrossRefGoogle Scholar
Léger, A., Puget, J.L., 1984, Astron. Astrophys., 137, L5 Google Scholar
Pruppacher, H.R., Klett, J.D., 1978, Microphysics of Clouds and Precipitation, D. Reidel Publ. Comp., Dordrecht CrossRefGoogle Scholar
Rossi, S.C.F., Benevides-Soaies, P., 1988, Astron. Astrophys., 192, 379 Google Scholar
Salpeter, E.E., 1977, Ann. Rev. Astron. Astrophys., 15, 267 CrossRefGoogle Scholar
Sedlmayr, E., 1989, In: Allamandola, L.J. & Tielens, A.G.G.M. (eds.), Interstellar Dust, Proc. IAU Symp. No. 135, D. Reidel Publ Comp., Dordrecht, p.467 CrossRefGoogle Scholar
Sharp, C.M., Huebner, W.F., 1990, Astrophys. J. Suppl, 72, 417 CrossRefGoogle Scholar
Tielens, A.G.G.M., 1989, In: Allamandola, L.J. & Tielens, A.G.G.M. (eds.), Interstellar Dust, Proc. IAU Symp. No. 135, D.Reidel Publ Comp., Dordrecht, p.239 CrossRefGoogle Scholar
Tielens, A.G.G.M., Allamandola, L.J., 1987, In: Morfill, G.E., Scholer, M. (eds.), Physical Processes in Interstellar Clouds, Proc. NATO Advanced Study Institute, D. Reidel Publ. Comp., Dordrecht, p.333 Google Scholar
Weinzierl, S., 1991, Diplomarbeit, Technische Universität, Berlin Google Scholar
Williams, D.A., 1989, In: Allamandola, L.J. & Tielens, A.G.G.M. (eds.), Interstellar Dust, Proc. IAU Symp. No. 135, D.Reidel Publ Comp., Dordrecht, p.367 CrossRefGoogle Scholar
Wright, E., 1989, In: Allamandola, L.J. & Tielens, A.G.G.M. (eds.), Interstellar Dust, Proc. IAU Symp. No. 135, D. Reidel Publ Comp., Dordrecht, p.337 CrossRefGoogle Scholar
Yamamoto, T., Nishida, S., 1977, Prog. Theor. Phys., 57, 1939 CrossRefGoogle Scholar