Synchrotron-Self Compton Spectral Evolution of PKS 2155-304
| dc.creator | Ciprini, Stefano | |
| dc.creator | Tosti, Gino | |
| dc.date | 2003-03-05 | |
| dc.date.accessioned | 2026-07-07T02:07:49Z | |
| dc.date.available | 2026-07-07T02:07:49Z | |
| dc.description | The high frequency peaked blazar PKS 2155-304 is one of the brightest and most intensively studied prototype of BL Lac objects. Gamma-rays from PKS 2155-304 have been detected from the MeV to TeV ranges. We computed a synchrotron self-Compton (SSC) model, based on the temporal behavior of the particles distribution, responsible for the high-energy emission. Using the available simultaneous multiwavelength data, we simulated the overall spectral energy distribution (SED) and the spectral variability of this source. | |
| dc.description | 4 pages, 6 PS figures, 1 table. Poster at the International Workshop "High Energy Blazar Astronomy" celebrating the 50th anniversary of Tuorla Observatory (Tuorla Observatory, Turku, Finland, 17-21 June 2002). Proceedings to be published in the PASP Conference Series, Eds. A. Sillanpaa, L. O. Takalo, and E. Valtaoja | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0303107 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0303107 | |
| dc.identifier | ASP Conf.Ser. 299 (2003) 269 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5821 | |
| dc.subject | Astrophysics | |
| dc.title | Synchrotron-Self Compton Spectral Evolution of PKS 2155-304 | |
| dc.type | text |