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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 06433naa a2201477 4500 | |
| 001 | oai:DiVA.org:su-80094 | |
| 003 | SwePub | |
| 008 | 120912s2012 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-800942 URI |
| 024 | 7 | a https://doi.org/10.1088/0004-637X/754/2/1142 DOI |
| 040 | a (SwePub)su | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Hayashida, M.4 aut |
| 245 | 1 0 | a THE STRUCTURE AND EMISSION MODEL OF THE RELATIVISTIC JET IN THE QUASAR 3C 279 INFERRED FROM RADIO TO HIGH-ENERGY gamma-RAY OBSERVATIONS IN 2008-2010 |
| 264 | 1 | c 2012 |
| 338 | a print2 rdacarrier | |
| 500 | a AuthorCount:93; | |
| 520 | a We present time-resolved broadband observations of the quasar 3C 279 obtained from multi-wavelength campaigns conducted during the first two years of the Fermi Gamma-ray Space Telescope mission. While investigating the previously reported gamma-ray/optical flare accompanied by a change in optical polarization, we found that the optical emission appears to be delayed with respect to the gamma-ray emission by about 10 days. X-ray observations reveal a pair of isolated flares separated by similar to 90 days, with only weak gamma-ray/optical counterparts. The spectral structure measured by Spitzer reveals a synchrotron component peaking in the mid-infrared band with a sharp break at the far-infrared band during the gamma-ray flare, while the peak appears in the millimeter (mm)/submillimeter (sub-mm) band in the low state. Selected spectral energy distributions are fitted with leptonic models including Comptonization of external radiation produced in a dusty torus or the broad-line region. Adopting the interpretation of the polarization swing involving propagation of the emitting region along a curved trajectory, we can explain the evolution of the broadband spectra during the gamma-ray flaring event by a shift of its location from similar to 1 pc to similar to 4 pc from the central black hole. On the other hand, if the gamma-ray flare is generated instead at sub-pc distance from the central black hole, the far-infrared break can be explained by synchrotron self-absorption. We also model the low spectral state, dominated by the mm/sub-mm peaking synchrotron component, and suggest that the corresponding inverse-Compton component explains the steady X-ray emission. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 653 | a galaxies: active | |
| 653 | a galaxies: jets | |
| 653 | a gamma rays: galaxies | |
| 653 | a quasars: individual (3C 279) | |
| 653 | a radiation mechanisms: non-thermal | |
| 653 | a X-rays: galaxies | |
| 700 | 1 | a Madejski, G. M.4 aut |
| 700 | 1 | a Nalewajko, K.4 aut |
| 700 | 1 | a Sikora, M.4 aut |
| 700 | 1 | a Wehrle, A. E.4 aut |
| 700 | 1 | a Ogle, P.4 aut |
| 700 | 1 | a Collmar, W.4 aut |
| 700 | 1 | a Larsson, Stefanu Stockholms universitet,Fysikum,Institutionen för astronomi4 aut0 (Swepub:su)slars |
| 700 | 1 | a Fukazawa, Y.4 aut |
| 700 | 1 | a Itoh, R.4 aut |
| 700 | 1 | a Chiang, J.4 aut |
| 700 | 1 | a Stawarz, L.4 aut |
| 700 | 1 | a Blandford, R. D.4 aut |
| 700 | 1 | a Richards, J. L.4 aut |
| 700 | 1 | a Max-Moerbeck, W.4 aut |
| 700 | 1 | a Readhead, A.4 aut |
| 700 | 1 | a Buehler, R.4 aut |
| 700 | 1 | a Cavazzuti, E.4 aut |
| 700 | 1 | a Ciprini, S.4 aut |
| 700 | 1 | a Gehrels, N.4 aut |
| 700 | 1 | a Reimer, A.4 aut |
| 700 | 1 | a Szostek, A.4 aut |
| 700 | 1 | a Tanaka, T.4 aut |
| 700 | 1 | a Tosti, G.4 aut |
| 700 | 1 | a Uchiyama, Y.4 aut |
| 700 | 1 | a Kawabata, K. S.4 aut |
| 700 | 1 | a Kino, M.4 aut |
| 700 | 1 | a Sakimoto, K.4 aut |
| 700 | 1 | a Sasada, M.4 aut |
| 700 | 1 | a Sato, S.4 aut |
| 700 | 1 | a Uemura, M.4 aut |
| 700 | 1 | a Yamanaka, M.4 aut |
| 700 | 1 | a Greiner, J.4 aut |
| 700 | 1 | a Kruehler, T.4 aut |
| 700 | 1 | a Rossi, A.4 aut |
| 700 | 1 | a Macquart, J. P.4 aut |
| 700 | 1 | a Bock, D. C. -J4 aut |
| 700 | 1 | a Villata, M.4 aut |
| 700 | 1 | a Raiteri, C. M.4 aut |
| 700 | 1 | a Agudo, I.4 aut |
| 700 | 1 | a Aller, H. D.4 aut |
| 700 | 1 | a Aller, M. F.4 aut |
| 700 | 1 | a Arkharov, A. A.4 aut |
| 700 | 1 | a Bach, U.4 aut |
| 700 | 1 | a Benitez, E.4 aut |
| 700 | 1 | a Berdyugin, A.4 aut |
| 700 | 1 | a Blinov, D. A.4 aut |
| 700 | 1 | a Blumenthal, K.4 aut |
| 700 | 1 | a Boettcher, M.4 aut |
| 700 | 1 | a Buemi, C. S.4 aut |
| 700 | 1 | a Carosati, D.4 aut |
| 700 | 1 | a Chen, W. P.4 aut |
| 700 | 1 | a Di Paola, A.4 aut |
| 700 | 1 | a Dolci, M.4 aut |
| 700 | 1 | a Efimova, N. V.4 aut |
| 700 | 1 | a Forne, E.4 aut |
| 700 | 1 | a Gomez, J. L.4 aut |
| 700 | 1 | a Gurwell, M. A.4 aut |
| 700 | 1 | a Heidt, J.4 aut |
| 700 | 1 | a Hiriart, D.4 aut |
| 700 | 1 | a Jordan, B.4 aut |
| 700 | 1 | a Jorstad, S. G.4 aut |
| 700 | 1 | a Joshi, M.4 aut |
| 700 | 1 | a Kimeridze, G.4 aut |
| 700 | 1 | a Konstantinova, T. S.4 aut |
| 700 | 1 | a Kopatskaya, E. N.4 aut |
| 700 | 1 | a Koptelova, E.4 aut |
| 700 | 1 | a Kurtanidze, O. M.4 aut |
| 700 | 1 | a Lahteenmaki, A.4 aut |
| 700 | 1 | a Lamerato, A.4 aut |
| 700 | 1 | a Larionov, V. M.4 aut |
| 700 | 1 | a Larionova, E. G.4 aut |
| 700 | 1 | a Larionova, L. V.4 aut |
| 700 | 1 | a Leto, P.4 aut |
| 700 | 1 | a Lindfors, E.4 aut |
| 700 | 1 | a Marscher, A. P.4 aut |
| 700 | 1 | a McHardy, I. M.4 aut |
| 700 | 1 | a Molina, S. N.4 aut |
| 700 | 1 | a Morozova, D. A.4 aut |
| 700 | 1 | a Nikolashvili, M. G.4 aut |
| 700 | 1 | a Nilsson, K.4 aut |
| 700 | 1 | a Reinthal, R.4 aut |
| 700 | 1 | a Roustazadeh, P.4 aut |
| 700 | 1 | a Sakamoto, T.4 aut |
| 700 | 1 | a Sigua, L. A.4 aut |
| 700 | 1 | a Sillanpaa, A.4 aut |
| 700 | 1 | a Takalo, L.4 aut |
| 700 | 1 | a Tammi, J.4 aut |
| 700 | 1 | a Taylor, B.4 aut |
| 700 | 1 | a Tornikoski, M.4 aut |
| 700 | 1 | a Trigilio, C.4 aut |
| 700 | 1 | a Troitsky, I. S.4 aut |
| 700 | 1 | a Umana, G.4 aut |
| 710 | 2 | a Stockholms universitetb Fysikum4 org |
| 773 | 0 | t Astrophysical Journalg 754:2, s. 114-q 754:2<114-x 0004-637Xx 1538-4357 |
| 856 | 4 | u https://arxiv.org/abs/1206.0745y arXiv:1206.0745 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-80094 |
| 856 | 4 8 | u https://doi.org/10.1088/0004-637X/754/2/114 |
Hitta mer i SwePub
- Av författaren/redakt...
- Hayashida, M.
- Madejski, G. M.
- Nalewajko, K.
- Sikora, M.
- Wehrle, A. E.
- Ogle, P.
- visa fler...
- Collmar, W.
- Larsson, Stefan
- Fukazawa, Y.
- Itoh, R.
- Chiang, J.
- Stawarz, L.
- Blandford, R. D.
- Richards, J. L.
- Max-Moerbeck, W.
- Readhead, A.
- Buehler, R.
- Cavazzuti, E.
- Ciprini, S.
- Gehrels, N.
- Reimer, A.
- Szostek, A.
- Tanaka, T.
- Tosti, G.
- Uchiyama, Y.
- Kawabata, K. S.
- Kino, M.
- Sakimoto, K.
- Sasada, M.
- Sato, S.
- Uemura, M.
- Yamanaka, M.
- Greiner, J.
- Kruehler, T.
- Rossi, A.
- Macquart, J. P.
- Bock, D. C. -J
- Villata, M.
- Raiteri, C. M.
- Agudo, I.
- Aller, H. D.
- Aller, M. F.
- Arkharov, A. A.
- Bach, U.
- Benitez, E.
- Berdyugin, A.
- Blinov, D. A.
- Blumenthal, K.
- Boettcher, M.
- Buemi, C. S.
- Carosati, D.
- Chen, W. P.
- Di Paola, A.
- Dolci, M.
- Efimova, N. V.
- Forne, E.
- Gomez, J. L.
- Gurwell, M. A.
- Heidt, J.
- Hiriart, D.
- Jordan, B.
- Jorstad, S. G.
- Joshi, M.
- Kimeridze, G.
- Konstantinova, T ...
- Kopatskaya, E. N ...
- Koptelova, E.
- Kurtanidze, O. M ...
- Lahteenmaki, A.
- Lamerato, A.
- Larionov, V. M.
- Larionova, E. G.
- Larionova, L. V.
- Leto, P.
- Lindfors, E.
- Marscher, A. P.
- McHardy, I. M.
- Molina, S. N.
- Morozova, D. A.
- Nikolashvili, M. ...
- Nilsson, K.
- Reinthal, R.
- Roustazadeh, P.
- Sakamoto, T.
- Sigua, L. A.
- Sillanpaa, A.
- Takalo, L.
- Tammi, J.
- Taylor, B.
- Tornikoski, M.
- Trigilio, C.
- Troitsky, I. S.
- Umana, G.
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