BL Lacertae: the multiwavelength campaign of 2000
| dc.creator | Ravasio, M. | |
| dc.creator | Tagliaferri, G. | |
| dc.creator | Ghisellini, G. | |
| dc.creator | Boettcher, M. | |
| dc.creator | Aller, H. D. | |
| dc.creator | Aller, M. F. | |
| dc.creator | Mang, O. | |
| dc.creator | Maraschi, L. | |
| dc.creator | Massaro, E. | |
| dc.creator | Raiteri, C. M. | |
| dc.creator | Villata, M. | |
| dc.creator | Teraesranta, H. | |
| dc.date | 2002-10-18 | |
| dc.date.accessioned | 2026-07-07T02:05:45Z | |
| dc.date.available | 2026-07-07T02:05:45Z | |
| dc.description | We present two BeppoSAX observations of BL Lacertae as part of a multiwavelength radio-to-TeV campaign. During the first observation we observe a faint Compton spectrum, while during the second, we detect a synchrotron spectrum with the highest [2-10] keV flux ever measured; above 10 keV an inverse Compton component begin to dominate. The synchrotron flux is very variable with time scales of 1 hr. We describe four different SED shifting the synchrotron peak both in frequency and flux intensity and we sketch a scenario in which a blob moves along a jet and can be located in or outside the BLR. This implies different radiative mechanism at work, SSC or external Compton, producing different high energy spectra. | |
| dc.description | 5 pages, 2 figures; to appear in the proccedings of the V Italian Conference on AGNs | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0210415 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0210415 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5198 | |
| dc.subject | Astrophysics | |
| dc.title | BL Lacertae: the multiwavelength campaign of 2000 | |
| dc.type | text |