A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Results of WEBT, VLBA and RXTE monitoring of 3C 279 during 2006-2007
Tekijät: Larionov VM, Jorstad SG, Marscher AP, Raiteri CM, Villata M, Agudo I, Aller MF, Arkharov AA, Asfandiyarov IM, Bach U, Bachev R, Berdyugin A, Bottcher M, Buemi CS, Calcidese P, Carosati D, Charlot P, Chen WP, Di Paola A, Dolci M, Dogru S, Doroshenko VT, Efimov YS, Erdem A, Frasca A, Fuhrmann L, Giommi P, Glowienka L, Gupta AC, Gurwell MA, Hagen-Thorn VA, Hsiao WS, Ibrahimov MA, Jordan B, Kamada M, Konstantinova TS, Kopatskaya EN, Kovalev YY, Kovalev YA, Kurtanidze OM, Lahteenmaki A, Lanteri L, Larionova LV, Leto P, Le Campion P, Lee CU, Lindfors E, Marilli E, McHardy I, Mingaliev MG, Nazarov SV, Nieppola E, Nilsson K, Ohlert J, Pasanen M, Porter D, Pursimo T, Ros JA, Sadakane K, Sadun AC, Sergeev SG, Smith N, Strigachev A, Sumitomo N, Takalo LO, Tanaka K, Trigilio C, Umana G, Ungerechts H, Volvach A, Yuan W
Kustantaja: EDP SCIENCES S A
Julkaisuvuosi: 2008
Tietokannassa oleva lehden nimi: ASTRONOMY & ASTROPHYSICS
Lehden akronyymi: ASTRON ASTROPHYS
Vuosikerta: 492
Numero: 2
Aloitussivu: 389
Lopetussivu: 400
Sivujen määrä: 12
ISSN: 0004-6361
DOI: https://doi.org/10.1051/0004-6361:200810937
Conclusions. The continuum spectrum agrees with steady injection of relativistic electrons with a power-law energy distribution of slope -3.2 that is steepened to -4.2 at high energies by radiative losses. The X- ray emission at flux minimum comes most likely from a new component that starts in an upstream section of the jet where inverse Compton scattering of seed photons from outside the jet is important. The rotation of the polarization vector implies that the jet contains a helical magnetic field that extends similar to 20 pc past the 43 GHz core.
