Hostname: page-component-7479d7b7d-pfhbr Total loading time: 0 Render date: 2024-07-12T14:02:57.556Z Has data issue: false hasContentIssue false
  • English
  • Français

The Structure of Galactic Nuclei: Recent Observations

Published online by Cambridge University Press:  30 March 2016

S. M. Faber
S. M. Faber*
Affiliation:
Lick Observatory and Board of Studies in Astronomy and Astrophysics, University of California, Santa Cruz

Extract

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.

Nuclei are often envisioned as sites for energetic and explosive phenomena in galaxies and may even be the birthplaces of quasars. Regardless of what models are chosen to represent such sources, a knowledge of the surrounding mass density and gravitational potential field is bound to be important for the creation and maintenance of the central engine. Moreover, galactic nuclei are worthy of close scrutiny even for their own sake. They constitute the brightest, most easily observed portions of galaxies and, in ellipticals, yield the central mass-to-light ratio, a quantity which cannot be determined for ellipticals using the ordinary rotation-curve method.

Type
Joint Discussion
Information
Highlights of Astronomy , Volume 5: Highlights of Astronomy. As presented at the XVIIth General Assembly of the IAU, 1979 , 1980 , pp. 135 - 142
Copyright
Copyright © Cambridge University Press 1980

References

Binney, J. 1979, preprint.Google Scholar
Davies, R.L. 1978, Ph.D. thesis, Cambridge University.Google Scholar
de Vaucouleurs, G. 1948, Ann. d’Ap., 11, 247.Google Scholar
de Vaucouleurs, G. 1953, M.N.R.A.S., 113, 134.CrossRefGoogle Scholar
de Vaucouleurs, G., and Capaccioli, M. 1979, preprint.Google Scholar
de Vaucouleurs, G., and Nieto, J.-L. 1979, Ap. J., 230, 697.CrossRefGoogle Scholar
Faber, S.M. and French, H. 1979, preprint.Google Scholar
Faber, S.M. and Gallagher, J.S. 1979, Ann. Rev. Astron. Ap. 17, in press.CrossRefGoogle Scholar
Faber, S.M. and Jackson, R.E. 1976, Ap. J., 204, 668.CrossRefGoogle Scholar
King, I.R. 1966, Astron. J., 71, 64.CrossRefGoogle Scholar
King, I.R. 1978, Ap. J., 222, 1.CrossRefGoogle Scholar
Kormendy, J. 1977, Ap. J., 218, 333.CrossRefGoogle Scholar
Light, E.S., Danlelson, R.E., and Schwarschild, M. 1974, Ap. J., 194, 257.CrossRefGoogle Scholar
Ruiz, M.T. 1976, Ap. J., 207, 382.CrossRefGoogle Scholar
Sargent, W.L.W., Young, P.J., Boksenberg, A., Shortridge, K., Lynds, C.R., and Hartwick, F.D.A. 1978, Ap. J., 221, 731.CrossRefGoogle Scholar
Schechter, P.L., and Gunn, J.E. 1979, Ap. J., 229, 472.CrossRefGoogle Scholar
Schweizer, F. 1979, preprint.Google Scholar
Spinrad, H., and Taylor, B.J. 1971, Ap. J. Suppl., 22, 445.Google Scholar
van den Bergh, S. 1979, Ap. J. Letters, 230, L161.CrossRefGoogle Scholar
Young, P.S., Sargent, W.L.W., Boksenberg, A., Lynds, C.R., and Hartwick, F.D.A. 1978, Ap. J., 222, 450.CrossRefGoogle Scholar