Hostname: page-component-7bb8b95d7b-pwrkn Total loading time: 0 Render date: 2024-10-02T22:29:17.105Z Has data issue: false hasContentIssue false
  • English
  • Français

Energy Sources and Physical Processes in Active Galaxies

Published online by Cambridge University Press:  25 May 2016

Daniel W. Weedman
Daniel W. Weedman*
Affiliation:
Department of Astronomy and Astrophysics, The Pennsylvania State University, State College, PA, 16802 USA

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.

The galaxy Markarian 231 is reviewed as a prototype that includes all physical processes associated with active galaxies. It contains both a starburst and an AGN which are highly obscured by dust. Its luminosity at various wavelengths is used to summarize how such a galaxy would appear at high redshift, as observed with missions such as HST, AXAF, and SIRTF. The conclusion is that Markarian 231 provides an excellent example for comparing low redshift and high redshift phenomena.

Type
III. AGN Theory and Models
Information
Symposium - International Astronomical Union , Volume 194: Activity in Galaxies and Related Phenomena , 1999 , pp. 191 - 198
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Baan, W.A., Haschick, A., & Henkel, C. 1992, AJ, 103, 728 CrossRefGoogle Scholar
Boksenberg, A., Carswell, R., Allen, D., Fosbury, R., Penston, M. & Sargent, W. 1977, MNRAS, 178, 451 Google Scholar
Carilli, C.L., Wrobel, J.M. & Ulvestad, J.S. 1998, AJ, 115, 928 CrossRefGoogle Scholar
Downes, D. & Solomon, P.M. 1998, ApJ, in press Google Scholar
Hamilton, D. & Keel, W. 1987, ApJ, 321, 211 Google Scholar
Huchra, J.P. 1977, ApJ, 217, 928 CrossRefGoogle Scholar
Hughes, D.H. et al., 1998, Nature, 394, 241 Google Scholar
Kawara, K. et al., 1998, A&A, in press Google Scholar
Khachikian, E. Ye. & Weedman, D.W. 1974, Ap.J., 192, 581 CrossRefGoogle Scholar
Kinney, A.L., Bohlin, R.C., Calzetti, D., Panagia, N. & Wyse, R.F.G. 1993, ApJS, 86, 5.Google Scholar
Krabbe, A., Colina, L. Thatte, N., & Kroker, H. 1997, ApJ, 476, 98 CrossRefGoogle Scholar
Lawrence, A., Elvis, M., Wilkes, B.J., McHardy, I., & Brandt, N. 1997, MNRAS, 285, 879 Google Scholar
Lipari, S., Colina, L. & Macchetto, F. 1994, ApJ, 427, 174 Google Scholar
Lowenthal, J.D. et al. 1997, ApJ, 481, 673 Google Scholar
Madau, P., Ferguson, H.C., Dickinson, M.E., Giavalisco, M., Steidel, C.C. & Fruchter, A. 1996, MNRAS, 283, 1388 CrossRefGoogle Scholar
Meurer, G.R., Heckman, T.M., Leitherer, C., Kinney, A., Robert, C., & Garnett, D.R. 1995, AJ, 110, 2665.CrossRefGoogle Scholar
Meurer, G., Heckman, T., Leitherer, C., Lowenthal, J., & Lehnert, M. 1997, AJ, 114, 54.CrossRefGoogle Scholar
Miles, J.W., Houck, J.R., Hayward, T.L., & Ashby, M.L.N. 1996, ApJ, 465, 191 Google Scholar
Moorwood, A.F.M., Lutz, D., Oliva, E., Marconi, A., Netzer, H., Genzel, R., Sturm, E., & de Graauw, Th..Google Scholar
Pettini, M., Kellogg, M., Steidel, C.C., Dickinson, M., Adelberger, K.L., & Giavalisco, M. 1998, ApJ, in press Google Scholar
Sanders, D.B., Young, J.S., Scoville, N.Z., Soifer, B.T. & Danielson, G.E. 1987, ApJ, 312, L5.Google Scholar
Schmidt, M., Schneider, D.P., & Gunn, J.P. 1995, AJ, 110, 68 Google Scholar
Schmitt, H.R., Kinney, A.L., Calzetti, D., & Storchi-Bergmann, T. 1997, AJ, 114, 592 Google Scholar
Smith, H.E., Lonsdale, C.J., & Lonsdale, C.J. 1998, AJ, 492, 137 Google Scholar
Smith, M.G. 1983, in Proceedings of the 24th Liege Colloquium, Quasars and Gravitational Lenses, Liege: Institut d'Astrophysique, 4 Google Scholar
Smith, P.S., Schmidt, G.D., Allen, R.G. & Angel, J.R.P. 1995, ApJ, 444, 146 CrossRefGoogle Scholar
Turner, T.J. 1998, ApJ, in press Weedman 1986, Quasar Astronomy, Cambridge: Cambridge University Press, 107 Google Scholar
Weedman, D.W., Wolovitz, J.B., Bershady, M.A., & Schneider, D.P. 1998, AJ, 116, 1643 Google Scholar