Standard
Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1. / Krawczynski, Henric; Muleri, Fabio; Dovčiak, Michal; Veledina, Alexandra; Rodriguez Cavero, Nicole; Svoboda, Jiri; Ingram, Adam; Matt, Giorgio; Garcia, Javier A.; Loktev, Vladislav; Negro, Michela; Poutanen, Juri; Kitaguchi, Takao; Podgorný, Jakub; Rankin, John; Zhang, Wenda; Berdyugin, Andrei; Berdyugina, Svetlana V.; Bianchi, Stefano; Blinov, Dmitry; Capitanio, Fiamma; Di Lalla, Niccolò; Draghis, Paul; Fabiani, Sergio; Kagitani, Masato; Kravtsov, Vadim; Kiehlmann, Sebastian; Latronico, Luca; Lutovinov, Alexander A.; Mandarakas, Nikos; Marin, Frédéric; Marinucci, Andrea; Miller, Jon M.; Mizuno, Tsunefumi; Molkov, Sergey V.; Omodei, Nicola; Petrucci, Pierre-Olivier; Ratheesh, Ajay; Sakanoi, Takeshi; Semena, Andrei N.; Skalidis, Raphael; Soffitta, Paolo; Tennant, Allyn F.; Thalhammer, Phillipp; Tombesi, Francesco; Weisskopf, Martin C.; Wilms, Joern; Zhang, Sixuan; Agudo, Iván; Antonelli, Lucio A.; Bachetti, Matteo; Baldini, Luca; Baumgartner, Wayne H.; Bellazzini, Ronaldo; Bongiorno, Stephen D.; Bonino, Raffaella; Brez, Alessandro; Bucciantini, Niccolò; Castellano, Simone; Cavazzuti, Elisabetta; Ciprini, Stefano; Costa, Enrico; De Rosa, Alessandra; Del Monte, Ettore; Di Gesu, Laura; Di Marco, Alessandro; Donnarumma, Immacolata; Doroshenko, Victor; Ehlert, Steven R.; Enoto, Teruaki; Evangelista, Yuri; Ferrazzoli, Riccardo; Gunji, Shuichi; Hayashida, Kiyoshi; Heyl, Jeremy; Iwakiri, Wataru; Jorstad, Svetlana G.; Karas, Vladimir; Kolodziejczak, Jeffery J.; La Monaca, Fabio; Liodakis, Ioannis; Maldera, Simone; Manfreda, Alberto; Marscher, Alan P.; Marshall, Herman L.; Mitsuishi, Ikuyuki; Ng, Chi-Yung; O’Dell, Stephen L.; Oppedisano, Chiara; Papitto, Alessandro; Pavlov, George G.; Peirson, Abel L.; Perri, Matteo; Pesce-Rollins, Melissa; Pilia, Maura; Possenti, Andrea; Puccetti, Simonetta; Ramsey, Brian D.; Romani, Roger W.; Sgrò, Carmelo; Slane, Patrick; Spandre, Gloria; Tamagawa, Toru; Tavecchio, Fabrizio; Taverna, Roberto; Tawara, Yuzuru; Thomas, Nicholas E.; Trois, Alessio; Tsygankov, Sergey; Turolla, Roberto; Vink, Jacco; Wu, Kinwah; Xie, Fei; Zane, Silvia.
в:
Science, Том 378, № 6620, 2022, стр. 650-654.
Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
Harvard
Krawczynski, H, Muleri, F, Dovčiak, M, Veledina, A, Rodriguez Cavero, N, Svoboda, J, Ingram, A, Matt, G, Garcia, JA, Loktev, V, Negro, M, Poutanen, J, Kitaguchi, T, Podgorný, J, Rankin, J, Zhang, W, Berdyugin, A, Berdyugina, SV, Bianchi, S, Blinov, D, Capitanio, F, Di Lalla, N, Draghis, P, Fabiani, S, Kagitani, M, Kravtsov, V, Kiehlmann, S, Latronico, L, Lutovinov, AA, Mandarakas, N, Marin, F, Marinucci, A, Miller, JM, Mizuno, T, Molkov, SV, Omodei, N, Petrucci, P-O, Ratheesh, A, Sakanoi, T, Semena, AN, Skalidis, R, Soffitta, P, Tennant, AF, Thalhammer, P, Tombesi, F, Weisskopf, MC, Wilms, J, Zhang, S, Agudo, I, Antonelli, LA, Bachetti, M, Baldini, L, Baumgartner, WH, Bellazzini, R, Bongiorno, SD, Bonino, R, Brez, A, Bucciantini, N, Castellano, S, Cavazzuti, E, Ciprini, S, Costa, E, De Rosa, A, Del Monte, E, Di Gesu, L, Di Marco, A, Donnarumma, I, Doroshenko, V, Ehlert, SR, Enoto, T, Evangelista, Y, Ferrazzoli, R, Gunji, S, Hayashida, K, Heyl, J, Iwakiri, W
, Jorstad, SG, Karas, V, Kolodziejczak, JJ, La Monaca, F, Liodakis, I, Maldera, S, Manfreda, A, Marscher, AP, Marshall, HL, Mitsuishi, I, Ng, C-Y, O’Dell, SL, Oppedisano, C, Papitto, A, Pavlov, GG, Peirson, AL, Perri, M, Pesce-Rollins, M, Pilia, M, Possenti, A, Puccetti, S, Ramsey, BD, Romani, RW, Sgrò, C, Slane, P, Spandre, G, Tamagawa, T, Tavecchio, F, Taverna, R, Tawara, Y, Thomas, NE, Trois, A, Tsygankov, S, Turolla, R, Vink, J, Wu, K, Xie, F & Zane, S 2022, '
Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1',
Science, Том. 378, № 6620, стр. 650-654.
https://doi.org/10.1126/science.add5399APA
Krawczynski, H., Muleri, F., Dovčiak, M., Veledina, A., Rodriguez Cavero, N., Svoboda, J., Ingram, A., Matt, G., Garcia, J. A., Loktev, V., Negro, M., Poutanen, J., Kitaguchi, T., Podgorný, J., Rankin, J., Zhang, W., Berdyugin, A., Berdyugina, S. V., Bianchi, S., ... Zane, S. (2022).
Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1.
Science,
378(6620), 650-654.
https://doi.org/10.1126/science.add5399Vancouver
Author
Krawczynski, Henric ; Muleri, Fabio ; Dovčiak, Michal ; Veledina, Alexandra ; Rodriguez Cavero, Nicole ; Svoboda, Jiri ; Ingram, Adam ; Matt, Giorgio ; Garcia, Javier A. ; Loktev, Vladislav ; Negro, Michela ; Poutanen, Juri ; Kitaguchi, Takao ; Podgorný, Jakub ; Rankin, John ; Zhang, Wenda ; Berdyugin, Andrei ; Berdyugina, Svetlana V. ; Bianchi, Stefano ; Blinov, Dmitry ; Capitanio, Fiamma ; Di Lalla, Niccolò ; Draghis, Paul ; Fabiani, Sergio ; Kagitani, Masato ; Kravtsov, Vadim ; Kiehlmann, Sebastian ; Latronico, Luca ; Lutovinov, Alexander A. ; Mandarakas, Nikos ; Marin, Frédéric ; Marinucci, Andrea ; Miller, Jon M. ; Mizuno, Tsunefumi ; Molkov, Sergey V. ; Omodei, Nicola ; Petrucci, Pierre-Olivier ; Ratheesh, Ajay ; Sakanoi, Takeshi ; Semena, Andrei N. ; Skalidis, Raphael ; Soffitta, Paolo ; Tennant, Allyn F. ; Thalhammer, Phillipp ; Tombesi, Francesco ; Weisskopf, Martin C. ; Wilms, Joern ; Zhang, Sixuan ; Agudo, Iván ; Antonelli, Lucio A. ; Bachetti, Matteo ; Baldini, Luca ; Baumgartner, Wayne H. ; Bellazzini, Ronaldo ; Bongiorno, Stephen D. ; Bonino, Raffaella ; Brez, Alessandro ; Bucciantini, Niccolò ; Castellano, Simone ; Cavazzuti, Elisabetta ; Ciprini, Stefano ; Costa, Enrico ; De Rosa, Alessandra ; Del Monte, Ettore ; Di Gesu, Laura ; Di Marco, Alessandro ; Donnarumma, Immacolata ; Doroshenko, Victor ; Ehlert, Steven R. ; Enoto, Teruaki ; Evangelista, Yuri ; Ferrazzoli, Riccardo ; Gunji, Shuichi ; Hayashida, Kiyoshi ; Heyl, Jeremy ; Iwakiri, Wataru
; Jorstad, Svetlana G. ; Karas, Vladimir ; Kolodziejczak, Jeffery J. ; La Monaca, Fabio ; Liodakis, Ioannis ; Maldera, Simone ; Manfreda, Alberto ; Marscher, Alan P. ; Marshall, Herman L. ; Mitsuishi, Ikuyuki ; Ng, Chi-Yung ; O’Dell, Stephen L. ; Oppedisano, Chiara ; Papitto, Alessandro ; Pavlov, George G. ; Peirson, Abel L. ; Perri, Matteo ; Pesce-Rollins, Melissa ; Pilia, Maura ; Possenti, Andrea ; Puccetti, Simonetta ; Ramsey, Brian D. ; Romani, Roger W. ; Sgrò, Carmelo ; Slane, Patrick ; Spandre, Gloria ; Tamagawa, Toru ; Tavecchio, Fabrizio ; Taverna, Roberto ; Tawara, Yuzuru ; Thomas, Nicholas E. ; Trois, Alessio ; Tsygankov, Sergey ; Turolla, Roberto ; Vink, Jacco ; Wu, Kinwah ; Xie, Fei ; Zane, Silvia. /
Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1. в:
Science. 2022 ; Том 378, № 6620. стр. 650-654.
BibTeX
@article{e996507217fc479bb85d925c2a075175,
title = "Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1",
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. A black hole in a binary system can rip material off of its companion star, which heats up and forms an accretion disk. The disc emits light in the optical and x-ray bands, forming an x-ray binary (XRB) system. Some XRBs also launch a jet of fast-moving material that is visible at radio wavelengths. Krawczynski et al. observed the x-ray polarization of Cygnus X-1, a black hole XRB with a radio jet. By comparing the measured polarization properties with several competing XRB models, they eliminated some hypothesized geometries and determined that the x-ray?emitting region extends parallel to the accretion disc. ?KTS x-ray polarization measurements determine the geometric arrangement of hot material accreting onto a black hole.",
author = "Henric Krawczynski and Fabio Muleri and Michal Dov{\v c}iak and Alexandra Veledina and {Rodriguez Cavero}, Nicole and Jiri Svoboda and Adam Ingram and Giorgio Matt and Garcia, {Javier A.} and Vladislav Loktev and Michela Negro and Juri Poutanen and Takao Kitaguchi and Jakub Podgorn{\'y} and John Rankin and Wenda Zhang and Andrei Berdyugin and Berdyugina, {Svetlana V.} and Stefano Bianchi and Dmitry Blinov and Fiamma Capitanio and {Di Lalla}, Niccol{\`o} and Paul Draghis and Sergio Fabiani and Masato Kagitani and Vadim Kravtsov and Sebastian Kiehlmann and Luca Latronico and Lutovinov, {Alexander A.} and Nikos Mandarakas and Fr{\'e}d{\'e}ric Marin and Andrea Marinucci and Miller, {Jon M.} and Tsunefumi Mizuno and Molkov, {Sergey V.} and Nicola Omodei and Pierre-Olivier Petrucci and Ajay Ratheesh and Takeshi Sakanoi and Semena, {Andrei N.} and Raphael Skalidis and Paolo Soffitta and Tennant, {Allyn F.} and Phillipp Thalhammer and Francesco Tombesi and Weisskopf, {Martin C.} and Joern Wilms and Sixuan Zhang and Iv{\'a}n Agudo and Antonelli, {Lucio A.} and Matteo Bachetti and Luca Baldini and Baumgartner, {Wayne H.} and Ronaldo Bellazzini and Bongiorno, {Stephen D.} and Raffaella Bonino and Alessandro Brez and Niccol{\`o} Bucciantini and Simone Castellano and Elisabetta Cavazzuti and Stefano Ciprini and Enrico Costa and {De Rosa}, Alessandra and {Del Monte}, Ettore and {Di Gesu}, Laura and {Di Marco}, Alessandro and Immacolata Donnarumma and Victor Doroshenko and Ehlert, {Steven R.} and Teruaki Enoto and Yuri Evangelista and Riccardo Ferrazzoli and Shuichi Gunji and Kiyoshi Hayashida and Jeremy Heyl and Wataru Iwakiri and Jorstad, {Svetlana G.} and Vladimir Karas and Kolodziejczak, {Jeffery J.} and {La Monaca}, Fabio and Ioannis Liodakis and Simone Maldera and Alberto Manfreda and Marscher, {Alan P.} and Marshall, {Herman L.} and Ikuyuki Mitsuishi and Chi-Yung Ng and O{\textquoteright}Dell, {Stephen L.} and Chiara Oppedisano and Alessandro Papitto and Pavlov, {George G.} and Peirson, {Abel L.} and Matteo Perri and Melissa Pesce-Rollins and Maura Pilia and Andrea Possenti and Simonetta Puccetti and Ramsey, {Brian D.} and Romani, {Roger W.} and Carmelo Sgr{\`o} and Patrick Slane and Gloria Spandre and Toru Tamagawa and Fabrizio Tavecchio and Roberto Taverna and Yuzuru Tawara and Thomas, {Nicholas E.} and Alessio Trois and Sergey Tsygankov and Roberto Turolla and Jacco Vink and Kinwah Wu and Fei Xie and Silvia Zane",
note = "doi: 10.1126/science.add5399",
year = "2022",
doi = "10.1126/science.add5399",
language = "English",
volume = "378",
pages = "650--654",
journal = "Science",
issn = "0036-8075",
publisher = "American Association for the Advancement of Science",
number = "6620",
}
RIS
TY - JOUR
T1 - Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1
AU - Krawczynski, Henric
AU - Muleri, Fabio
AU - Dovčiak, Michal
AU - Veledina, Alexandra
AU - Rodriguez Cavero, Nicole
AU - Svoboda, Jiri
AU - Ingram, Adam
AU - Matt, Giorgio
AU - Garcia, Javier A.
AU - Loktev, Vladislav
AU - Negro, Michela
AU - Poutanen, Juri
AU - Kitaguchi, Takao
AU - Podgorný, Jakub
AU - Rankin, John
AU - Zhang, Wenda
AU - Berdyugin, Andrei
AU - Berdyugina, Svetlana V.
AU - Bianchi, Stefano
AU - Blinov, Dmitry
AU - Capitanio, Fiamma
AU - Di Lalla, Niccolò
AU - Draghis, Paul
AU - Fabiani, Sergio
AU - Kagitani, Masato
AU - Kravtsov, Vadim
AU - Kiehlmann, Sebastian
AU - Latronico, Luca
AU - Lutovinov, Alexander A.
AU - Mandarakas, Nikos
AU - Marin, Frédéric
AU - Marinucci, Andrea
AU - Miller, Jon M.
AU - Mizuno, Tsunefumi
AU - Molkov, Sergey V.
AU - Omodei, Nicola
AU - Petrucci, Pierre-Olivier
AU - Ratheesh, Ajay
AU - Sakanoi, Takeshi
AU - Semena, Andrei N.
AU - Skalidis, Raphael
AU - Soffitta, Paolo
AU - Tennant, Allyn F.
AU - Thalhammer, Phillipp
AU - Tombesi, Francesco
AU - Weisskopf, Martin C.
AU - Wilms, Joern
AU - Zhang, Sixuan
AU - Agudo, Iván
AU - Antonelli, Lucio A.
AU - Bachetti, Matteo
AU - Baldini, Luca
AU - Baumgartner, Wayne H.
AU - Bellazzini, Ronaldo
AU - Bongiorno, Stephen D.
AU - Bonino, Raffaella
AU - Brez, Alessandro
AU - Bucciantini, Niccolò
AU - Castellano, Simone
AU - Cavazzuti, Elisabetta
AU - Ciprini, Stefano
AU - Costa, Enrico
AU - De Rosa, Alessandra
AU - Del Monte, Ettore
AU - Di Gesu, Laura
AU - Di Marco, Alessandro
AU - Donnarumma, Immacolata
AU - Doroshenko, Victor
AU - Ehlert, Steven R.
AU - Enoto, Teruaki
AU - Evangelista, Yuri
AU - Ferrazzoli, Riccardo
AU - Gunji, Shuichi
AU - Hayashida, Kiyoshi
AU - Heyl, Jeremy
AU - Iwakiri, Wataru
AU - Jorstad, Svetlana G.
AU - Karas, Vladimir
AU - Kolodziejczak, Jeffery J.
AU - La Monaca, Fabio
AU - Liodakis, Ioannis
AU - Maldera, Simone
AU - Manfreda, Alberto
AU - Marscher, Alan P.
AU - Marshall, Herman L.
AU - Mitsuishi, Ikuyuki
AU - Ng, Chi-Yung
AU - O’Dell, Stephen L.
AU - Oppedisano, Chiara
AU - Papitto, Alessandro
AU - Pavlov, George G.
AU - Peirson, Abel L.
AU - Perri, Matteo
AU - Pesce-Rollins, Melissa
AU - Pilia, Maura
AU - Possenti, Andrea
AU - Puccetti, Simonetta
AU - Ramsey, Brian D.
AU - Romani, Roger W.
AU - Sgrò, Carmelo
AU - Slane, Patrick
AU - Spandre, Gloria
AU - Tamagawa, Toru
AU - Tavecchio, Fabrizio
AU - Taverna, Roberto
AU - Tawara, Yuzuru
AU - Thomas, Nicholas E.
AU - Trois, Alessio
AU - Tsygankov, Sergey
AU - Turolla, Roberto
AU - Vink, Jacco
AU - Wu, Kinwah
AU - Xie, Fei
AU - Zane, Silvia
N1 - doi: 10.1126/science.add5399
PY - 2022
Y1 - 2022
N2 - 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. A black hole in a binary system can rip material off of its companion star, which heats up and forms an accretion disk. The disc emits light in the optical and x-ray bands, forming an x-ray binary (XRB) system. Some XRBs also launch a jet of fast-moving material that is visible at radio wavelengths. Krawczynski et al. observed the x-ray polarization of Cygnus X-1, a black hole XRB with a radio jet. By comparing the measured polarization properties with several competing XRB models, they eliminated some hypothesized geometries and determined that the x-ray?emitting region extends parallel to the accretion disc. ?KTS x-ray polarization measurements determine the geometric arrangement of hot material accreting onto a black hole.
AB - 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. A black hole in a binary system can rip material off of its companion star, which heats up and forms an accretion disk. The disc emits light in the optical and x-ray bands, forming an x-ray binary (XRB) system. Some XRBs also launch a jet of fast-moving material that is visible at radio wavelengths. Krawczynski et al. observed the x-ray polarization of Cygnus X-1, a black hole XRB with a radio jet. By comparing the measured polarization properties with several competing XRB models, they eliminated some hypothesized geometries and determined that the x-ray?emitting region extends parallel to the accretion disc. ?KTS x-ray polarization measurements determine the geometric arrangement of hot material accreting onto a black hole.
U2 - 10.1126/science.add5399
DO - 10.1126/science.add5399
M3 - Article
VL - 378
SP - 650
EP - 654
JO - Science
JF - Science
SN - 0036-8075
IS - 6620
ER -
