Gamma rays from cloud penetration at the base of AGN jets

被引：64

作者：

Araudo, A. T. ^{[1
,2
,4
]}

Bosch-Ramon, V. ^{[3
]}

Romero, G. E. ^{[1
,2
]}

机构：

[1] Inst Argentino Radioastron, RA-1894 Buenos Aires, DF, Argentina

[2] Univ Nacl La Plata, Fac Ciencias Astron & Geofis, RA-1900 La Plata, Buenos Aires, Argentina

[3] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany

[4] Consejo Nacl Invest Cient & Tecn, RA-1033 Buenos Aires, DF, Argentina

来源：

ASTRONOMY & ASTROPHYSICS | 2010年 / 522卷

关键词：

quasars: general; radiation mechanisms: non-thermal; gamma rays: general; BROAD-LINE REGION; ACTIVE GALACTIC NUCLEI; HIGH-ENERGY EMISSION; CENTAURUS-A; COSMIC-RAYS; BLACK-HOLE; RADIO; ACCELERATION; VARIABILITY; LUMINOSITY;

D O I：

10.1051/0004-6361/201014660

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Context. Dense and cold clouds seem to populate the broad line region surrounding the central black hole in AGNs. These clouds may interact with the AGN jet base which could have observational consequences. Aims. We study the gamma-ray emission produced by these jet-cloud interactions, and explore the conditions under which this radiation would be detectable. Methods. We investigate the hydrodynamical properties of jet-cloud interactions and the resulting shocks, and develop a model to compute the spectral energy distribution of the emission generated by the particles accelerated in these shocks. We discuss our model in the context of radio-loud AGNs, with applications to two representative cases, the low-luminous Centaurus A and the powerful 3C 273. Results. Some fraction of the jet power may be channelled into gamma-ray energy, which is likely to be dominated by synchrotron self-Compton radiation, and have typical variability timescales similar to the cloud lifetime within the jet, which is longer than several hours. Many clouds can interact with the jet simultaneously leading to fluxes significantly higher than in one interaction, but then variability will be smoothed out. Conclusions. Jet-cloud interactions may produce detectable gamma-rays in non-blazar AGNs that are transient in nearby low-luminous sources such as Cen A, and steady in the case of powerful objects of FR II type.

引用

页数：8

共 59 条

[1] THE FIRST CATALOG OF ACTIVE GALACTIC NUCLEI DETECTED BY THE FERMI LARGE AREA TELESCOPE [J].

Abdo, A. A. ;

Ackermann, M. ;

Ajello, M. ;

Allafort, A. ;

Antolini, E. ;

Atwood, W. B. ;

Axelsson, M. ;

Baldini, L. ;

Ballet, J. ;

Barbiellini, G. ;

Bastieri, D. ;

Baughman, B. M. ;

Bechtol, K. ;

Bellazzini, R. ;

Berenji, B. ;

Blandford, R. D. ;

Bloom, E. D. ;

Bogart, J. R. ;

Bonamente, E. ;

Borgland, A. W. ;

Bouvier, A. ;

Bregeon, J. ;

Brez, A. ;

Brigida, M. ;

Bruel, P. ;

Buehler, R. ;

Burnett, T. H. ;

Buson, S. ;

Caliandro, G. A. ;

Cameron, R. A. ;

Cannon, A. ;

Caraveo, P. A. ;

Carrigan, S. ;

Casandjian, J. M. ;

Cavazzuti, E. ;

Cecchi, C. ;

Celik, Oe. ;

Celotti, A. ;

Charles, E. ;

Chekhtman, A. ;

Chen, A. W. ;

Cheung, C. C. ;

Chiang, J. ;

Ciprini, S. ;

Claus, R. ;

Cohen-Tanugi, J. ;

Conrad, J. ;

Costamante, L. ;

Cotter, G. ;

Cutini, S. .

ASTROPHYSICAL JOURNAL, 2010, 715 (01) :429-457

[2]

ABDO AA, 2009, APJ, V713, P1310

[3] Particle acceleration by ultrarelativistic shocks: theory and simulations [J].

Achterberg, A ;

Gallant, YA ;

Kirk, JG ;

Guthmann, AW .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2001, 328 (02) :393-408

[4] DISCOVERY OF VERY HIGH ENERGY γ-RAY EMISSION FROM CENTAURUS A WITH HESS [J].

Aharonian, F. ;

Akhperjanian, A. G. ;

Anton, G. ;

de Almeida, U. Barres ;

Bazer-Bachi, A. R. ;

Becherini, Y. ;

Behera, B. ;

Benbow, W. ;

Bernloehr, K. ;

Boisson, C. ;

Bochow, A. ;

Borrel, V. ;

Brion, E. ;

Brucker, J. ;

Brun, P. ;

Buehler, R. ;

Bulik, T. ;

Buesching, I. ;

Boutelier, T. ;

Chadwick, P. M. ;

Charbonnier, A. ;

Chaves, R. C. G. ;

Cheesebrough, A. ;

Chounet, L. -M. ;

Clapson, A. C. ;

Coignet, G. ;

Dalton, M. ;

Daniel, M. K. ;

Davids, I. D. ;

Degrange, B. ;

Deil, C. ;

Dickinson, H. J. ;

Djannati-Atai, A. ;

Domainko, W. ;

Drury, L. O'C. ;

Dubois, F. ;

Dubus, G. ;

Dyks, J. ;

Dyrda, M. ;

Egberts, K. ;

Emmanoulopoulos, D. ;

Espigat, P. ;

Farnier, C. ;

Feinstein, F. ;

Fiasson, A. ;

Foerster, A. ;

Fontaine, G. ;

Fuessling, M. ;

Gabici, S. ;

Gallant, Y. A. .

ASTROPHYSICAL JOURNAL LETTERS, 2009, 695 (01) :L40-L44

[5] Proton-synchrotron radiation of large-scale jets in active galactic nuclei [J].

Aharonian, FA .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2002, 332 (01) :215-230

[6] Searching for the hidden broad-line region in Centaurus A [J].

Alexander, DM ;

Hough, JH ;

Young, S ;

Bailey, JA ;

Heisler, CA ;

Lumsden, SL ;

Robinson, A .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1999, 303 (02) :L17-L22

[7] High-energy emission from jet-clump interactions in microquasars [J].

Araudo, A. T. ;

Bosch-Ramon, V. ;

Romero, G. E. .

ASTRONOMY & ASTROPHYSICS, 2009, 503 (03) :673-681

[8] HIGH-ENERGY EMISSION FROM JET-CLOUD INTERACTIONS IN AGNs [J].

Araudo, Anabella T. ;

Bosch-Ramon, Valenti ;

Romero, Gustavo E. .

INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2010, 19 (06) :931-936

[9]

ARAUDO AT, 2010, IJMPD IN PRESS

[10] Gamma-rays from interactions of stars with active galactic nucleus jets [J].

Bednarek, W ;

Protheroe, RJ .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1997, 287 (03) :L9-L13

← 1 2 3 4 5 6 →