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Soft X-Ray Properties of a Complete Sample of Radio Sources

Published online by Cambridge University Press:  25 May 2016

J. Siebert ,
W. Brinkmann ,
R. Morganti ,
C.N. Tadhunter ,
I.J. Danziger ,
R.A.E. Fosbury  and
S. Di Serego Alighieri
J. Siebert
Affiliation:
1 MPE - Giessenbachstrasse, D-85740 Garching, Germany
W. Brinkmann
Affiliation:
1 MPE - Giessenbachstrasse, D-85740 Garching, Germany
R. Morganti
Affiliation:
2 IRA - CNR, via Gobetti 101, I-40129 Bologna, Italy
C.N. Tadhunter
Affiliation:
4 Physics Department, University of Sheffield, Sheffield S3, UK
I.J. Danziger
Affiliation:
5 ESO, Karl Schwarzschild Str. 2, D-85748 Garching, Germany
R.A.E. Fosbury
Affiliation:
6 ST-ECF, Karl Schwarzschild Str.2, D-85748 Garching, Germany
S. Di Serego Alighieri
Affiliation:
8 OA - Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy

Abstract

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We investigate the X–ray properties of a complete sample of 88 radio sources derived from the Wall & Peacock 2–Jy sample. We find that Lx correlates well with core radio luminosity for all object classes, whereas the Lx – Ltotal is probably introduced by sample selection effects. Further, evidence for an anisotropic X–ray component in broad line radio galaxies is reported. A full description of the results will be given elsewhere (Siebert et al. 1996).

Type
Relation between Radio and Other Wavelenghts
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 263 - 264
Copyright
Copyright © Kluwer 1996 

References

Akritas, M.G., Siebert, J., 1996, MNRAS , in press Google Scholar
Siebert, J., Brinkmann, W., Morganti, R., Tadhunter, C.N., Danziger, I.J., Fosbury, R.A.E., di Serego Alighieri, S., 1996, MNRAS , in press Google Scholar