Abstract
The properties of compact extragalactic radio sources are investigated using a sample of 27 sources extensively observed at millimeter frequencies. It is suggested that the radio variability of all AGN, independent of their classification, can be understood in terms of growing and decaying shocks in a jet.
Preview
Unable to display preview. Download preview PDF.
References
Altschüler, D.R.: Astron. J. 87, 387 (1982)
Edelson, R.A.: Astron. J. 94, 1150 (1987)
Kühr, H., et al.: Astron. Astrophys. Suppl. 45, 367 (1981)
Marscher, A.P., Gear, W.K.: Astrophys. J. 298, 114 (1985)
Salonen, E., et al.: Astron. Astrophys. Suppl. 51, 47
Valtaoja, E., et al.: Astron. Astrophys. 203, 1 (1988)
Wardle, J.F.C,et al.: Astron. J. 86, 848 (1981)
Author information
Authors and Affiliations
Editor information
Rights and permissions
Copyright information
© 1989 Springer-Verlag
About this paper
Cite this paper
Valtaoja, E., Lainela, M., Teräsranta, H. (1989). Radio variability of BL Lacs and related objects: Observations vs. shocked jet models. In: Maraschi, L., Maccacaro, T., Ulrich, M.H. (eds) BL Lac Objects. Lecture Notes in Physics, vol 334. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0031143
Download citation
DOI: https://doi.org/10.1007/BFb0031143
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-51389-6
Online ISBN: 978-3-540-46203-3
eBook Packages: Springer Book Archive