Abstract
More than 50 sources have been detected by EGRET in 4 years of operations (e.g. von Montigny et al. 1995). Almost all of them show the violent characteristics typical of blazars, such as superluminal motions, strong radio emission mainly produced in a flat spectrum core and large amplitude variability at all frequencies. Interestingly, optical polarization does not seem to be required, since more than 1/3 of the detected sources are less than 3% polarized.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Blandford, R.D. & Levinson, A. 1995, ApJ, 441, 79
Dermer, C., Schlickeiser, R. & Mastichiadis, A. 1992, A & A, 256, L27
Dondi, L. & Ghisellini, G. 1995, MNRAS, 273, 583
Ghisellini, G. & Madau, P., 1995, submitted to MNRAS
Ghisellini, G., Maraschi, L. & Dondi, L., 1995, Third Compton Symp., A & ASS, in press
Maraschi, L., Ghisellini, G. & Celotti, A. 1992, ApJ, 397, L5
Maraschi, L., et al. 1994, ApJ, 435, L91
Sikora, M., Begelman, M.C. & Rees, M.J. 1994, ApJ, 421, 153
von Montigny, C., et al. 1995, ApJ, 440, 525
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1996 International Astronomical Union
About this paper
Cite this paper
Ghisellini, G. (1996). X-Ray and Gamma-Ray Emission in Blazars. In: Ekers, R., Fanti, C., Padrielli, L. (eds) Extragalactic Radio Sources. International Astronomical Union, vol 175. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0295-4_146
Download citation
DOI: https://doi.org/10.1007/978-94-009-0295-4_146
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-4122-2
Online ISBN: 978-94-009-0295-4
eBook Packages: Springer Book Archive