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Grain Evolution in the Framework of Disk-Halo Interactions

Published online by Cambridge University Press:  03 August 2017

F. Ferrini
F. Ferrini*
Affiliation:
Dipartimento di Fisica Università di Pisa 56100 Pisa, Italy

Abstract

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The presence of dust grains at high galactic latitude as well as in the Halo of external galaxies has received substantial observative support in the last few years. Besides intense hydrodynamics stirring phenomena, like supernovae expanding shells, stellar winds and Galactic fountains, the removal of dust from the Disk can be ascribed to the global galactic radiation field. The continuous sputtering in the hot Halo gas may explain the large scale height found for refractory elements (Edgar and Savage, 1989).

Type
III. Theory and Modelling
Information
Symposium - International Astronomical Union , Volume 144: The Interstellar Disk-Halo Connection in Galaxies , 1991 , pp. 397 - 406
Copyright
Copyright © Kluwer 1991 

References

REFERENCES

Barsella, B., Ferrini, F., Greenberg, J. M., and Aiello, S. 1989 Astr. Ap. , 209, 349.Google Scholar
Burstein, D., Rubin, V.C.: 1985, Ap. J. , 297, 423 CrossRefGoogle Scholar
Burton, W.B.: 1990, in Chemical and Dynamical Evolution of Galaxies , eds. Ferrini, F., Franco, J. and Matteucci, F., Giardini, Pisa, p.657 Google Scholar
Chiao, R.Y., and Wickramasinge, N.C. 1972, M.N.R.A.S. , 159, 361.CrossRefGoogle Scholar
Cochran, W. D., and Ostriker, J. P. 1977, Ap. J. , 211, 392.CrossRefGoogle Scholar
Désert, F. X., Bazell, D., and Boulanger, F. 1988, Ap. J. , 334, 815.CrossRefGoogle Scholar
Divari, , and Reznova, , 1970 Sov. Astron.,. Google Scholar
Draine, B. T. 1987, Princeton Obs. POP-213.Google Scholar
Draine, B. T., and Lee, H. M. 1984, Ap. J. , 285, 89.CrossRefGoogle Scholar
Draine, B. T., and Salpeter, E. E. 1979, Ap. J. , 231, 77.CrossRefGoogle Scholar
Edgar, R. J., and Savage, B. D. 1989, Ap. J. , 340, 762.CrossRefGoogle Scholar
Elmegreen, B. G., and Chiang, W. H. 1982, Ap. J. , 253, 666.CrossRefGoogle Scholar
Ferrara, A., Ferrini, F., Barsella, B. and Aiello, S. 1990, Astr. Ap. , in press Google Scholar
Ferrara, A., Franco, J., Ferrini, F., and Barsella, B. 1989, IAU Colloquium 120, Structure and Dynamics of the Interstellar Medium , eds. Moles, M. and Tenorio-Tagle, G., Springer Verlag, Berlin, p.454.CrossRefGoogle Scholar
Ferrini, F., Barsella, B., Greenberg, J.M. 1988, Dust in the Universe , eds. Bailey, M.E. and Williams, D.A., Cambridge Univ. Press, p.513 Google Scholar
Franco, J., and Cox, D. P. 1986, P. A. S. P. , 98, 1076.CrossRefGoogle Scholar
Franco, J., Ferrini, F., Ferrara, A., and Barsella, B. 1990, Ap. J. , in press Google Scholar
Greenberg, J.M., Chlewicki, G., 1983, Ap. J. , 272, 563 CrossRefGoogle Scholar
Greenberg, J.M., Ferrini, F., Barsella, B., Aiello, S., 1987, Nature , 327, 214 CrossRefGoogle Scholar
Herter, T., Shupe, D.L., and Chernoff, D.F. 1990, Ap. J. , 325, 149.CrossRefGoogle Scholar
Krishna Swamy, K. S., and O'Dell, C. R. 1967, Ap. J. , 147, 529.CrossRefGoogle Scholar
Kwok, S. 1975, Ap. J. , 198, 583.CrossRefGoogle Scholar
Mathews, W. G. 1967, Ap. J. , 147, 965.CrossRefGoogle Scholar
Mathis, J. S., Rumpl, W., and Nordsiek, K. H. 1977, Ap. J. , 217, 425 CrossRefGoogle Scholar
Mathis, J. S., Mezger, P. G., and Panagia, N. 1983, Astr. Ap. , 128, 212.Google Scholar
O'Dell, C. R., York, D. G., and Henize, K. G. 1967, Ap. J. , 150, 835.CrossRefGoogle Scholar
Pecker, J.-C.: 1972, Astr. Ap. , 18, 253 Google Scholar
Pecker, J.-C. 1974, Astr. Ap. , 35, 7.Google Scholar
Pence, W. 1976, Ap.J. , 203, 39 CrossRefGoogle Scholar
Phillip, H.L.: 1977, Phys. Rev. , B16, 2896 CrossRefGoogle Scholar
Rand, R.J., Kulkarni, S.R., and Hester, J.J. 1990, Ap. J. , 325, L1.CrossRefGoogle Scholar
Rohlfs, R., Herbstmeier, U., Mebold, U., and Winneberg, A. 1989, Astr. Ap. 211, 402.Google Scholar
Rudnicki, K., Wszolek, B., Masi, S., De Bernardis, P., and Salvi, A. 1989, Comm. in Ap. , 13, 171 Google Scholar
Salpeter, E. E. 1974, Ap. J. , 193, 585.CrossRefGoogle Scholar
Savage, B.D. 1989, in Evolution of the Interstellar Medium, P.A.S.P , in press Google Scholar
Sofue, Y. 1987, Publ. Astr. Soc. Jap. , 39, 547.Google Scholar
Spitzer, L. 1941, Ap. J. , 94, 232.CrossRefGoogle Scholar
Spitzer, L. 1978, Physical Processes in the Interstellar Medium , (New York: Wiley and Sons).Google Scholar
Tosatti, E., Bassani, F.: 1970, Nuovo Cimento , 65B, 161 CrossRefGoogle Scholar
van Albada, T.S., Bahcall, J.N., Begeman, K., Sancisi, R.: 1985, Ap. J. , 295, 305 CrossRefGoogle Scholar
Véron-Cetty, M.P. and Véron, P. 1985, Astr. Ap. , 145, 425.Google Scholar
Wevers, B.M.H.R.: 1984, Ph. D. Thesis, Groningen University Google Scholar
Wolfe, B., Routly, P., Wightman, A., and Spitzer, L. 1950, Phys. Rev. , 79, 1020.CrossRefGoogle Scholar
Yoshii, Y., and Takahara, F. 1988, Ap.J. , 326, 1 CrossRefGoogle Scholar