Aviso: para depositar documentos, por favor, inicia sesión e identifícate con tu cuenta de correo institucional de la UCM con el botón MI CUENTA UCM. No emplees la opción AUTENTICACIÓN CON CONTRASEÑA
 

Black hole lightning due to particle acceleration at subhorizon scales

dc.contributor.authorAntoranz Canales, Pedro
dc.contributor.authorBarrio Uña, Juan Abel
dc.contributor.authorContreras González, José Luis
dc.contributor.authorFonseca González, María Victoria
dc.contributor.authorLópez Moya, Marcos
dc.contributor.authorMiranda Pantoja, José Miguel
dc.contributor.authorSatalecka, Konstanzja
dc.contributor.authorScapin, Valeria
dc.date.accessioned2023-06-19T13:29:52Z
dc.date.available2023-06-19T13:29:52Z
dc.date.issued2014-11-28
dc.description© The authors. We would like to thank the Instituto de Astrofísica de Canarias for the excellent working conditions at the Observatorio del Roque de los Muchachos in La Palma. The support of the German BMBF and MPG, the Italian INFN, the Swiss National Fund SNF, and the Spanish MICINN is gratefully acknowledged. This work was also supported by the CPAN CSD2007-00042 and MultiDark CSD2009-00064 projects of the Spanish Consolider-Ingenio 2010 programme, by grant 127740 of the Academy of Finland, by the DFG Cluster of Excellence “Origin and Structure of the Universe”, by the Croatian Science Foundation (HrZZ) Projects 09/176, by the University of Rijeka Project 13.12.1.3.02, by the DFG Collaborative Research Centers SFB823/C4 and SFB876/C3, and by the Polish MNiSzW grant 745/N-ESSMAGIC/2010/0. We thank also the support by DFG WI 1860/10-1. J. S. was supported by ERDF and the Spanish MINECO through FPA2012-39502 and JCI-2011-10019 grants. E. R. was partially supported by the Spanish MINECO projects AYA2009-13036-C02-02 and AYA2012-38491-C02-01 and by the Generalitat Valenciana project PROMETEO/2009/104, as well as by the COST MP0905 action "Black Holes in a Violent Universe". The European VLBI Network is a joint facility of European, Chinese, South African and other radio astronomy institutes funded by their national research councils. The research leading to these results has received funding from the European Commission Seventh Framework Programme (FP/2007-2013) under grant agreement No. 283393 (RadioNet3). The MAGIC data is archived in the data center at the Port d´Informació Científica (PIC) in Barcelona. The EVN data are available at the Data Archive at the Joint Institute for VLBI in Europe (JIVE).
dc.description.abstractSupermassive black holes with masses of millions to billions of solar masses are commonly found in the centers of galaxies. Astronomers seek to image jet formation using radio interferometry, but still suffer from insufficient angular resolution. An alternative method to resolve small structures is to measure the time variability of their emission. Here, we report on gamma-ray observations of the radio galaxy IC 310 obtained with the MAGIC telescopes revealing variability with doubling time scales faster than 4.8 min. Causality constrains the size of the emission region to be smaller than 20% of the gravitational radius of its central black hole. We suggest that the emission is associated with pulsar-like particle acceleration by the electric field across a magnetospheric gap at the base of the radio jet.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipUnión Europea. FP7
dc.description.sponsorshipGerman BMBF
dc.description.sponsorshipGerman MPG
dc.description.sponsorshipItalian INFN
dc.description.sponsorshipSwiss National Fund SNF
dc.description.sponsorshipSpanish MICINN
dc.description.sponsorshipSpanish Consolider-Ingenio 2010 programme
dc.description.sponsorshipAcademy of Finland
dc.description.sponsorshipDFG Cluster of Excellence “Origin and Structure of the Universe”
dc.description.sponsorshipCroatian Science Foundation (HrZZ
dc.description.sponsorshipUniversity of Rijeka
dc.description.sponsorshipDFG Collaborative Research Centers
dc.description.sponsorshipPolish MNiSzW
dc.description.sponsorshipERDF
dc.description.sponsorshipSpanish MINECO
dc.description.sponsorshipGeneralitat Valenciana
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/29124
dc.identifier.doi10.1126/science.1256183
dc.identifier.issn0036-8075
dc.identifier.officialurlhttp://dx.doi.org/10.1126/science.1256183
dc.identifier.relatedurlhttp://www.sciencemag.org/
dc.identifier.relatedurlhttp://arxiv.org/abs/1412.4936
dc.identifier.urihttps://hdl.handle.net/20.500.14352/33871
dc.issue.number6213
dc.journal.titleScience
dc.language.isoeng
dc.page.final1084
dc.page.initial1080
dc.publisherAmer Assoc Advancement Science
dc.relation.projectIDFP/2007-2013 RadioNet3 (283393)
dc.relation.projectIDCPAN CSD2007- 00042
dc.relation.projectIDCSD2009-00064
dc.relation.projectID127740
dc.relation.projectID09/176
dc.relation.projectID13.12.1.3.02
dc.relation.projectIDSFB823/C4
dc.relation.projectIDSFB876/C3
dc.relation.projectID745/N-ESSMAGIC/2010/0
dc.relation.projectIDDFG WI 1860/10-1.
dc.relation.projectIDFPA2012-39502
dc.relation.projectIDJCI-2011-10019
dc.relation.projectIDAYA2009-13036-C02-02
dc.relation.projectIDCOST MP0905
dc.relation.projectIDPROMETEO/2009/104
dc.relation.projectIDCOST MP0905
dc.rights.accessRightsopen access
dc.subject.cdu537
dc.subject.cdu539.1
dc.subject.keywordGamma-ray emission
dc.subject.keywordActive galactic nuclei
dc.subject.keywordFast TEV variability
dc.subject.keywordGalaxy IC 310
dc.subject.keywordRelativistic jets
dc.subject.keywordEnergy
dc.subject.keywordM87
dc.subject.keywordBlazars
dc.subject.keywordFlare
dc.subject.keywordPKS-2155-304.
dc.subject.ucmElectricidad
dc.subject.ucmElectrónica (Física)
dc.subject.ucmFísica nuclear
dc.subject.unesco2202.03 Electricidad
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleBlack hole lightning due to particle acceleration at subhorizon scales
dc.typejournal article
dc.volume.number346
dcterms.references1. R. D. Blandford, A. Königl, ApJ, 232, 34 (1979). 2. L. Maraschi, G. Ghisellini, A. Celotti, ApJ, 397, L5 (1992). 3. C. D. Dermer, R. Schlickeiser, ApJ, 416, 458 (1993). 4. R. D. Blandford, R.L. Znajek, MNRAS, 179, 433 (1977). 5. S. van Velzen, H. Falcke, A&A, 557, L7 (2013). 6. A. P. Marscher, W. K. Gear, ApJ, 298, 114 (1985). 7. S. S. Doeleman, et al., Science, 338, 355 (2012). 8. I. Vovk, A. Neronov, ApJ, 767, 103 (2013). 9. J. Albert, et al., ApJ, 685, L23 (2008). 10. A. Abramowski, et al., ApJ, 746, 151 (2012) 11. K. Gebhardt, J. Thomas, ApJ, 700, 1690 (2009). 12. V. A. Acciari, et al., Science, 325, 444 (2009). 13. J. Albert, et al., ApJ, 669, 862 (2007). 14. F. Aharonian, et al., ApJ, 664, L71 (2007). 15. M. C. Begelman, A. C. Fabian, M. J. Rees, MNRAS, 384, L19 (2008). 16. In special relativity, the Lorentz and Doppler factors are defined as Γj = (1 − β2)−1/2 and δ = [Γj(1 − β cos θ)]−1, respectively, where β denotes the dimensionless shock velocity and θ the angle between the line of sight and the direction of the jet, ignoring the cosmological (1 + z) factor. The apparent bolometric luminosity differs from its isotropic comoving-frame value by the factor δ 4. 17. M. L. Lister, et al., AJ, 138, 1874 (2009). 18. C. M. Urry, P. Padovani, M. Stickel, ApJ, 382, 501 (1991). 19. M. Lyutikov, M. Lister, Ap, 722, 197 (2010). 20. G. Ghisellini, F. Tavecchio, MNRAS, 386, L28 (2008). 21. D. Giannios, D. A. Uzdensky, M. C. Begelman, MNRAS, 395, L29 (2009). 22. F. C. Michel, Physical Review Letters, 23, 247 (1969). 23. M. Lyutikov, MNRAS, 396, 1545 (2009). 24. J. G. Kirk, I. Mochol, ApJ, 729, 104 (2011). 25. J. Aleksić, et al., Astroparticle Physics, 35, 435 (2012). 26. A. Neronov, D. Semikov, I. Vovk, A&A, 519, L6 (2010). 27. J. Aleksić, et al., ApJ, 723, L207 (2010). 28. J. Aleksić, et al., A&A, 563, A91 (2014). 29. K. Gültekin, et al., ApJ 698, 198 (2009). 30. D. B. McElroy, ApJS, 100, 105 (1995). 31. A. Merloni, S. Heinz, T. di Matteo, MNRAS, 345, 1057 (2003). 32. M. Kadler, et al., A&A, 538, L1 (2012). 33. D. Giannios, D. A. Uzdensky, M. C. Begelman, MNRAS, 402, 1649 (2010). 34. W. Bednarek, R. J. Protheroe, MNRAS, 287, L9 (1997). 35. M. V. Barkov, F. A. Aharonian, V. Bosch-Ramon, ApJ, 724, 1517 (2010). 36. M. V. Barkov, V. Bosch-Ramon, F. A. Aharonian, ApJ, 755, 170 (2012). 37. F. M. Rieger, K. Mannheim, A&A, 353, 473 (2000). 38. A. Neronov, F. A. Aharonian, ApJ, 671, 85 (2007). 39. A. Y. Neronov, D. V. Semikoz, I. I. Tkachev, New Journal of Physics, 11, 065015 (2009). 40. A. Levinson, F. Rieger, ApJ, 730, 123 (2011). 41. V. S. Beskin, Y. N. Istomin, V. I. Parev, SOVAST, 36, 642 (1992).
dspace.entity.typePublication
relation.isAuthorOfPublication6bc87e5f-9b77-4982-b112-0d4f8aa128d0
relation.isAuthorOfPublication11e5fd8b-1a86-4f8d-85c6-135541232be4
relation.isAuthorOfPublication6a14529e-a65e-4709-9bc1-61f9429841c1
relation.isAuthorOfPublication9f2c0e34-0edd-497a-bbd0-fbd9d348e85c
relation.isAuthorOfPublication8b5d96d7-bd11-4ee4-87d0-258a1e077e26
relation.isAuthorOfPublication328f9716-2012-44f9-aacc-ef8d48782a77
relation.isAuthorOfPublication.latestForDiscovery6bc87e5f-9b77-4982-b112-0d4f8aa128d0

Download

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
AntoranzP09preprint.pdf
Size:
376.78 KB
Format:
Adobe Portable Document Format

Collections