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DC Field | Value | Language |
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dc.contributor.author | Böttcher, M | - |
dc.date.accessioned | 2008-05-29T07:04:42Z | - |
dc.date.available | 2008-05-29T07:04:42Z | - |
dc.date.issued | 2002 | - |
dc.identifier.citation | BASI, Vol. 30, No. 1, pp. 115 - 124 | en |
dc.identifier.uri | http://hdl.handle.net/2248/2374 | - |
dc.description.abstract | The current status of leptonic jet models for blazars is reviewed. Differences between the quasar and BL-Lac subclasses of blazars may be understood in terms of the dominance of difference radiation mechanisms in the gamma-ray regime. Spectral variability patterns of different blazar subclasses appear to be significantly different and require different intrinsic mechanisms causing gamma-ray flares. As examples, recent results of long-term multiwavelength monitoring of PKS 0528-134, 3C 279, and Mrk 501 are interpreted in the framework of leptonic jet models. Short-term variability patterns give important additional clues about the source geometry and the relevant radiation mechanisms in blazars. Challenges for future observational efforts are discussed. | en |
dc.format.extent | 1110824 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Astronomical Society of India | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/2002BASI...30..115B | en |
dc.subject | Active Galaxies | en |
dc.subject | Extragalactic Jets | en |
dc.subject | Radiation Mechanisms | en |
dc.title | Physics input from multiwavelength observations of AGN | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
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Bottcher.pdf | 1.08 MB | Adobe PDF | View/Open |
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