Comparative Study of Extragalactic Radio Sources from “Double Jet” Models

  • H. Dole
  • H. Sol
  • L. Vicente
Conference paper
Part of the International Astronomical Union book series (IAUS, volume 175)


It seems now important to consider bulk velocity gradients inside jets (Blandford, 1993; Biretta et al, 1995) and recent results from tomography technique suggest the presence of different components in radio sources (Rudnick, this symposium). A few jet models take explicitly into account two components with different bulk velocities (Smith, Raine, 1985; Baker et al, 1988; Sol et al, 1989; Achatz et al, 1990). A fast beam comes from the vicinity of the black hole while a slower collimated wind is emitted by the accretion disk. When stable, the two components can survive along the jet. If a fast instability develops at a distance D c from core, the beam is destroyed over some relaxation length. Its energy and momentum are transmitted to the wind. Apparent change in the flow regime such as slowing down, decollimation, local bending or discontinuity in surface brightness is the expected observational signature of such critical zones on radio maps. The exact appearance of the zone depends on the parameters of the two flows and on their interaction regime.


Black Hole Radio Source Accretion Disk Critical Zone Alfven Wave 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


  1. Achatz, U., Lesch, H., Schlickeiser, 1990, AA, 233, 391.ADSGoogle Scholar
  2. Baker, D.N., Borovsky, J.E., Benford, G., Eilek, J.A., 1988, ApJ, 326, 110.ADSCrossRefGoogle Scholar
  3. Biretta, J.A., Zhou, F., Owen, F.N., 1995, ApJ, 447, 582.ADSCrossRefGoogle Scholar
  4. Blandford, R., 1993, Astrophysical jets, Space Telescope Science Institute Symposium Series, Burgarella, D., Livio, M., O’Dea, C.P., eds, Cambridge University Press, p. 15.Google Scholar
  5. Smith, M.D., Raine, D.J., 1985, MNRAS, 212, 425 ADSGoogle Scholar
  6. Sol, H., Pelletier, G., Asséo, E., 1989, MNRAS, 237 , 411 ADSzbMATHGoogle Scholar

Copyright information

© International Astronomical Union 1996

Authors and Affiliations

  • H. Dole
    • 1
  • H. Sol
    • 1
  • L. Vicente
    • 1
  1. 1.Observatoire de Paris-MeudonDARC, UPR176 du CNRSFrance

Personalised recommendations