TeV Blazars - Observations and Models
| dc.creator | Krawczynski, Henric | |
| dc.date | 2003-09-16 | |
| dc.date.accessioned | 2026-07-07T10:47:41Z | |
| dc.date.available | 2026-07-07T10:47:41Z | |
| dc.description | Since the first TeV blazar Markarian (Mrk) 421 was detected in 1992, the number of established TeV gamma-ray emitting BL Lac objects has grown to 6, with redshifts ranging from 0.031 (Mrk 421) to 0.129 (H 1426+428). The intensive study of these sources has had a major impact on our understanding of the blazar phenomenon. The most notable observational results have been extremely fast large amplitude flux and spectral variability on hour time scales, and a pronounced X-ray - TeV gamma-ray flux correlation. In this paper we discuss recent observational results and report on progress in their theoretical interpretation. | |
| dc.description | Accepted for publication in New Astronomy Reviews; Invited Talk at the "2nd VERITAS Symposium on TeV Astrophysics of Extragalactic Sources", April 24-26, 2003, Chicago; 8 Pages, 2 Figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0309443 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0309443 | |
| dc.identifier | NewAstron.Rev.48:367-373,2004 | |
| dc.identifier | doi:10.1016/j.newar.2003.12.008 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/183621 | |
| dc.subject | Astrophysics | |
| dc.title | TeV Blazars - Observations and Models | |
| dc.type | text |