Hostname: page-component-78c5997874-t5tsf Total loading time: 0 Render date: 2024-11-19T05:15:29.109Z Has data issue: false hasContentIssue false
  • English
  • Français

Radio structure and the IR-UV spectra of quasars

Published online by Cambridge University Press:  19 July 2016

Beverley J. Wills  and
D. Wills
Beverley J. Wills
Affiliation:
McDonald Observatory and Department of Astronomy, University of Texas, RLM 15.308, Austin, Texas 78712, U.S.A.
D. Wills
Affiliation:
McDonald Observatory and Department of Astronomy, University of Texas, RLM 15.308, Austin, Texas 78712, U.S.A.

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.

Here we present two main results that relate properties of quasar IR-to-UV spectra to the fraction of radio flux density in the compact core.

Type
II. Continuum Emission
Information
Symposium - International Astronomical Union , Volume 119: Quasars , 1986 , pp. 215 - 216
Copyright
Copyright © Reidel 1986 

References

Boroson, T.A., Persson, S.E., and Oke, J.B. 1985, Ap. J., 293, 120.CrossRefGoogle Scholar
Orr, M.J.L. and Browne, I.W.A. 1982, M.N.R.A.S., 200, 1067.CrossRefGoogle Scholar
Steiner, J.E. 1981, Ap. J., 250, 469.CrossRefGoogle Scholar
Wills, B.J. and Browne, I.W.A. 1986, Ap. J., March 1.Google Scholar