Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-26T20:18:10.538Z Has data issue: false hasContentIssue false
  • English
  • Français

Symmetric Ejection of Massive Objects from Galactic Nuclei

Published online by Cambridge University Press:  14 August 2015

M. J. Valtonen
M. J. Valtonen*
Affiliation:
Institute of Astronomy, Cambridge, England Research Institute for Theoretical Physics, Helsinki, Finland

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

It is shown that massive objects can be ejected symmetrically in two opposite directions from the nucleus of a giant elliptical galaxy only under special initial conditions. A way of obtaining these conditions is outlined, and the resulting picture of evolution of galactic nuclei, including a quasar or a Seyfert galaxy phase, is shown to be compatible with observations.

Type
Part III/Nuclei
Information
Symposium - International Astronomical Union , Volume 69: Dynamics of Stellar Systems , 1975 , pp. 395 - 403
Copyright
Copyright © Reidel 1975 

References

Arp, H. C.: 1967, Astrophys. Letters 1, 1.Google Scholar
Bignell, R. C.: 1973, Astron. J. 78, 557.CrossRefGoogle Scholar
Branson, N. J. B. A., Elsmore, B., Pooley, G. G., and Ryle, M.: 1972, Monthly Notices Roy. Astron. Soc. 156, 377.CrossRefGoogle Scholar
Daltabuit, E. and Cox, D.: 1972, Astrophys. J. Letters 173, L13.CrossRefGoogle Scholar
Felten, J. E., Arp, H. C., and Lynds, C. R.: 1970, Astrophys. J. 159, 415.CrossRefGoogle Scholar
Graham, I.: 1970, Monthly Notices Roy. Astron. Soc. 149, 319.CrossRefGoogle Scholar
Hiltner, W. A., 1959, Astrophys. J. 130, 340.CrossRefGoogle Scholar
Hohl, F.: 1971, Astrophys. J. 168, 343.CrossRefGoogle Scholar
Kellermann, K. I., Clark, B. G., Shaffer, D. B., Cohen, M. H., Jauncey, D. L., Broderick, J. J., and Niell, A. E.: 1974, Astrophys. J. Letters, 189, L19.CrossRefGoogle Scholar
Knapp, G. R. and Kerr, F. J.: 1974, Astron. J. 79, 667.CrossRefGoogle Scholar
Legg, T. H., Broten, N. W., Fort, D. N., Yen, J. L., Bale, F. V., Barber, P. C., and Quigley, M. J. S.: 1973, Nature Phys. Sci. 244, 18.CrossRefGoogle Scholar
Matthews, T. A., Morgan, W. W., and Schmidt, M.: 1964, Astrophys. J. 140, 35.CrossRefGoogle Scholar
Miley, G. K.: 1971, Monthly Notices Roy. Astron. Soc. 152, 477.CrossRefGoogle Scholar
Osterbrock, D. E.: 1971, Pontificiae Academiae Scientiarum, Scripta Varia No. 35, p. 151.Google Scholar
Ostriker, J. P. and Peebles, P. J. E.: 1973, Astrophys. J. 186, 467.CrossRefGoogle Scholar
Salpeter, E. E.: 1971, Nature Phys. Sci. 233, 5.CrossRefGoogle Scholar
Saslaw, W. C., Valtonen, M. J., and Aarseth, S. J.: 1974, Astrophys. J. 190, 253.CrossRefGoogle Scholar
Searle, L.: 1965, Nature Phys. Sci. 207, 1282.CrossRefGoogle Scholar
Shklovskii, I. S.: 1972, Soviet Astron. 16, 193.Google Scholar
Turland, B. D.: 1975, in press.Google Scholar
Walker, M. F.: 1968, Astrophys. Letters 2, 65.Google Scholar
Walker, M. F. and Hayes, S.: 1967, Astrophys. J. 149, 481.CrossRefGoogle Scholar