Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1
Files
First author draft
Date
2022-11-11
Authors
Krawczynski, Henric
Muleri, Fabio
Dovčiak, Michal
Veledina, Alexandra
Rodriguez Cavero, Nicole
Svoboda, Jiri
Ingram, Adam
Matt, Giorgio
Garcia, Javier A.
Loktev, Vladislav
Version
OA Version
First author draft
Citation
H. Krawczynski, F. Muleri, M. Dovčiak, A. Veledina, N. Rodriguez Cavero, J. Svoboda, A. Ingram, G. Matt, J.A. Garcia, V. Loktev, M. Negro, J. Poutanen, T. Kitaguchi, J. Podgorný, J. Rankin, W. Zhang, A. Berdyugin, S.V. Berdyugina, S. Bianchi, D. Blinov, F. Capitanio, N. Di Lalla, P. Draghis, S. Fabiani, M. Kagitani, V. Kravtsov, S. Kiehlmann, L. Latronico, A.A. Lutovinov, N. Mandarakas, F. Marin, A. Marinucci, J.M. Miller, T. Mizuno, S.V. Molkov, N. Omodei, P.-O. Petrucci, A. Ratheesh, T. Sakanoi, A.N. Semena, R. Skalidis, P. Soffitta, A.F. Tennant, P. Thalhammer, F. Tombesi, M.C. Weisskopf, J. Wilms, S. Zhang, I. Agudo, L.A. Antonelli, M. Bachetti, L. Baldini, W.H. Baumgartner, R. Bellazzini, S.D. Bongiorno, R. Bonino, A. Brez, N. Bucciantini, S. Castellano, E. Cavazzuti, S. Ciprini, E. Costa, A. De Rosa, E. Del Monte, L. Di Gesu, A. Di Marco, I. Donnarumma, V. Doroshenko, S.R. Ehlert, T. Enoto, Y. Evangelista, R. Ferrazzoli, S. Gunji, K. Hayashida, J. Heyl, W. Iwakiri, S.G. Jorstad, V. Karas, J.J. Kolodziejczak, F. La Monaca, I. Liodakis, S. Maldera, A. Manfreda, A.P. Marscher, H.L. Marshall, I. Mitsuishi, C.-Y. Ng, S.L. O'Dell, C. Oppedisano, A. Papitto, G.G. Pavlov, A.L. Peirson, M. Perri, M. Pesce-Rollins, M. Pilia, A. Possenti, S. Puccetti, B.D. Ramsey, R.W. Romani, C. Sgrò, P. Slane, G. Spandre, T. Tamagawa, F. Tavecchio, R. Taverna, Y. Tawara, N.E. Thomas, A. Trois, S. Tsygankov, R. Turolla, J. Vink, K. Wu, F. Xie, S. Zane. 2022. "Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1." Science, Volume 378, Issue 6620, pp.650-654. https://doi.org/10.1126/science.add5399
Abstract
A black hole x-ray binary (XRB) system forms when gas is stripped from a normal star and accretes onto a black hole, which heats the gas sufficiently to emit x-rays. We report a polarimetric observation of the XRB Cygnus X-1 using the Imaging X-ray Polarimetry Explorer. The electric field position angle aligns with the outflowing jet, indicating that the jet is launched from the inner x-ray-emitting region. The polarization degree is 4.01 ± 0.20% at 2 to 8 kiloelectronvolts, implying that the accretion disk is viewed closer to edge-on than the binary orbit. These observations reveal that hot x-ray-emitting plasma is spatially extended in a plane perpendicular to, not parallel to, the jet axis.