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The Gas Dynamics of Accretion

Published online by Cambridge University Press:  14 August 2015

E. A. Spiegel
E. A. Spiegel*
Affiliation:
Dept. of Astronomy, Columbia University, New York, N.Y., U.S.A.

Extract

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The term accretion originally referred, in astronomical contexts, to the capture of mass by stars, and, later, to mass capture by other centers of gravitational force. As such, the process has not proved to be of general importance, in spite of early hopes. However, there are other aspects of the problem which may yet prove worthy of attention in interstellar gas dynamics. In particular, the effects of stars, galaxies, or even clusters of galaxies, on ambient matter streaming by them may be detectable, directly or indirectly, and it is on such possible effects that I shall concentrate here. These effects are related to the original accretion problem but may be thought of separately; nevertheless, I retain the use of the term accretion to refer to all aspects of the motions induced in an ambient medium by a gravitating object.

Type
Part I: Description and General Theory of the Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 39: Interstellar Gas Dynamics , 1970 , pp. 201 - 214
Copyright
Copyright © Reidel 1970 

References

Benjamin, T. B. and Ellis, A. T.: 1966, Phil. Trans. Roy. Soc. London A260, 221.Google Scholar
* Bernstein, I. B. and Rabinowitz, : 1959, Phys. Fluids 2, 72.Google Scholar
Bondi, H.: 1952, Monthly Notices Roy. Astron. Soc. 112, 195.CrossRefGoogle Scholar
Bondi, H. and Hoyle, F.: 1944, Monthly Notices Roy. Astron. Soc. 104, 273.CrossRefGoogle Scholar
* Cohen, I. M.: 1963, Phys. Fluids 6, 1492.CrossRefGoogle Scholar
Danby, J. and Bray, T. A.: 1967, Astron. J. 12, 219.CrossRefGoogle Scholar
Danby, J. and Camm, G. L.: 1957, Monthly Notices Roy. Astron. Soc. 117, 50.CrossRefGoogle Scholar
* Davydov, B. and Zmanovskaya, L. J.: 1936, Zh. Tekhn. Fiz. 3, 215.Google Scholar
Dokuchaev, V. P.: 1964, Astron. Zh. 41, 33 (translation: 1964, Soviet Astron. 8, 23).Google Scholar
Eddington, S. A.: 1959, The Internal Constitution of the Stars, Dover Publications, New York, p. 391.Google Scholar
* Hester, S. D. and Sonin, A. A.: Sixth Rarefied Gas Dynamics Conference (no further information available).Google Scholar
Kraus, L. and Watson, K. M.: 1958, Phys. Fluids 1, 480.CrossRefGoogle Scholar
* Lam, S. H.: 1965, Phys. Fluids 8, 73.CrossRefGoogle Scholar
Landau, L. D. and Lifshitz, E. M.: 1960, Electrodynamics of Continuous Media, Pergamon Press, London.Google Scholar
* Langmuir, I. and Mott-Smith, H. M.: 1926, Phys. Rev. 28, 727.Google Scholar
Lyttleton, R. A.: 1953, The Comets and Their Origin, Cambridge University Press, p. 66.Google Scholar
McCrea, W. H.: 1955, IAU Symposium No. 2, Gas Dynamics of Cosmic Clouds, (ed. by van de Hulst, H. C. and Burgers, J. M.), North-Holland Publishing Company, Amsterdam, p. 186.Google Scholar
Mestel, L.: 1954, Monthly Notices Roy. Astron. Soc. 114, 437.CrossRefGoogle Scholar
Morgan, W. W., Strömgren, B. and Johnson, H. M.: 1955, Astrophys. J. 121, 611.CrossRefGoogle Scholar
Ozernoi, L. M. and Zasov, A. V. (in preparation).Google Scholar
Parker, E. N.: 1958, Astrophys. J. 128, 664.CrossRefGoogle Scholar
* Su, C. H. and Lam, S H.: 1963, Phys. Fluids 6, 1479.CrossRefGoogle Scholar
Ward, G. N.: 1955, Linearized Theory of High-Speed Flow, Cambridge University Press.Google Scholar
Weymann, R.: 1962, Astrophys. J. 136, 476.CrossRefGoogle Scholar
Wickramasinghe, N. C., Donn, B. D. and Stecher, T. P.: 1966, Astrophys. J. 146, 590.CrossRefGoogle Scholar