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DOI

  • 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
  • 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
  • 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
  • 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
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.
Язык оригиналаанглийский
DOI
СостояниеОтправлено - 23 окт 2024

    Области исследований

  • Astrophysics - High Energy Astrophysical Phenomena

ID: 126980727