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对 Mrk 421 开展的为期两周的 $IXPE$ 监测活动

A Two-Week $IXPE$ Monitoring Campaign on Mrk 421

W. Peter Maksym, Ioannis Liodakis, M. Lynne Saade, Dawoon E. Kim, Riccardo Middei, Laura Di Gesu, Sebastian Kiehlmann, Gabriele Matzeu, Iván Agudo, Alan P. Mars… 展开作者

W. Peter Maksym, Ioannis Liodakis, M. Lynne Saade, Dawoon E. Kim, Riccardo Middei, Laura Di Gesu, Sebastian Kiehlmann, Gabriele Matzeu, Iván Agudo, Alan P. Marscher, Steven R. Ehlert, Svetlana G. Jorstad, Philip Kaaret, Herman L. Marshall, Luigi Pacciani, Matteo Perri, Simonetta Puccetti, Pouya M. Kouch, Elina Lindfors, Francisco José Aceituno, Giacomo Bonnoli, Víctor Casanova, Juan Escudero, Beatriz Agís-González, César Husillos, Daniel Morcuende, Jorge Otero-Santos, Alfredo Sota, Vilppu Piirola, Ryo Imazawa, Mahito Sasada, Yasushi Fukazawa, Koji S. Kawabata, Makoto Uemura, Tsunefumi Mizuno, Tatsuya Nakaoka, Hiroshi Akitaya, Callum McCall, Helen E. Jermak, Iain A. Steele, George A. Borman, Tatiana S. Grishina, Vladimir A. Hagen-Thorn, Evgenia N. Kopatskaya, Elena G. Larionova, Daria A. Morozova, Sergey S. Savchenko, Ekaterina V. Shishkina, Ivan S. Troitskiy, Yulia V. Troitskaya, Andrey A. Vasilyev, Alexey V. Zhovtan, Ioannis Myserlis, Mark Gurwell, Garrett Keating, Ramprasad Rao, Colt Pauley, Emmanouil Angelakis, Alexander Kraus, Andrei V. Berdyugin, Masato Kagitani, Vadim Kravtsov, Juri Poutanen, Takeshi Sakanoi, Sincheol Kang, Sang-Sung Lee, Sang-Hyun Kim, Whee Yeon Cheong, Hyeon-Woo Jeong, Chanwoo Song, Dmitry Blinov, Elena Shablovinskaya, Lucio Angelo Antonelli, Matteo Bachetti, Luca Baldini, Wayne H. Baumgartner, Ronaldo Bellazzini, Stefano Bianchi, Stephen D. Bongiorno, Raffaella Bonino, Alessandro Brez, Niccoló Bucciantini, Fiamma Capitanio, Simone Castellano, Elisabetta Cavazzuti, Chien-Ting Chen, Stefano Ciprini, Enrico Costa, Alessandra De Rosa, Ettore Del Monte, Niccoló Di Lalla, Alessandro Di Marco, Immacolata Donnarumma, Victor Doroshenko, Michal Dovčiak, Teruaki Enoto, Yuri Evangelista, Sergio Fabiani, Riccardo Ferrazzoli, Javier A. Garcia, Shuichi Gunji, Kiyoshi Hayashida, Jeremy Heyl, Wataru Iwakiri, Vladimir Karas, Fabian Kislat, Takao Kitaguchi, Jeffery J. Kolodziejczak, Henric Krawczynski, Fabio La Monaca, Luca Latronico, Simone Maldera, Alberto Manfreda, Frédéric Marin, Andrea Marinucci, Francesco Massaro, Giorgio Matt, Ikuyuki Mitsuishi, Fabio Muleri, Michela Negro, C. -Y. Ng, Stephen L. O'Dell, Nicola Omodei, Chiara Oppedisano, Alessandro Papitto, George G. Pavlov, Abel Lawrence Peirson, Melissa Pesce-Rollins, Pierre-Olivier Petrucci, Maura Pilia, Andrea Possenti, Brian D. Ramsey, John Rankin, Ajay Ratheesh, Oliver J. Roberts, Roger W. Romani, Carmelo Sgró, Patrick Slane, Paolo Soffitta, Gloria Spandre, Douglas A. Swartz, Toru Tamagawa, Fabrizio Tavecchio, Roberto Taverna, Yuzuru Tawara, Allyn F. Tennant, Nicholas E. Thomas, Francesco Tombesi, Alessio Trois, Sergey S. Tsygankov, Roberto Turolla, Jacco Vink, Martin C. Weisskopf, Kinwah Wu, Fei Xie, Silvia Zane

AI总结:

该研究利用 IXPE 对耀变体 Mrk 421 进行两周密集X射线偏振监测,并结合射电与光学观测,揭示偏振角约90°旋转及能量相关变化,支持湍流磁场中的能量分层激波加速情景。

摘要:

X射线偏振是研究天体物理喷流中粒子加速的一种独特新探测手段,这一手段因 Imaging X-ray Polarimetry Explorer(成像X射线偏振探测器,IXPE)而成为可能。在此,我们报告针对耀变体 Mrk 421 的首次密集X射线偏振监测活动。我们的观测还配有一项更为密集的射电和光学偏振监测。我们发现X射线偏振度和偏振角均存在显著的短时标变化,其中包括绕喷流轴约 $90^\circ$ 的角度旋转。我们将其归因于磁场的随机变化;这与湍流的存在相符,但也不太可能仅由湍流解释。与此同时,较低能量的偏振度显著更低,并且至多表现出轻微变化。我们的监测活动为如下情景提供了进一步证据:相对论性电子的能量分层激波加速与湍流磁场相结合,共同导致了耀变体喷流中从光学到X射线的同步辐射。

英文摘要:

X-ray polarization is a unique new probe of the particle acceleration in astrophysical jets made possible through the Imaging X-ray Polarimetry Explorer. Here we report on the first dense X-ray polarization monitoring campaign on the blazar Mrk 421. Our observations were accompanied by an even denser radio and optical polarization campaign. We find significant short-timescale variability in both X-ray polarization degree and angle, including a $\sim90^\circ$ angle rotation about the jet axis. We attribute this to random variations of the magnetic field, consistent with the presence of turbulence but also unlikely to be explained by turbulence alone. At the same time, the degree of lower-energy polarization is significantly lower and shows no more than mild variability. Our campaign provides further evidence for a scenario in which energy-stratified shock-acceleration of relativistic electrons, combined with a turbulent magnetic field, is responsible for optical to X-ray synchrotron emission in blazar jets.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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