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.

In: Science, Vol. 378, No. 6620, 2022, p. 650-654.

Research output: Contribution to journalArticlepeer-review

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, vol. 378, no. 6620, pp. 650-654. https://doi.org/10.1126/science.add5399

APA

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.add5399

Vancouver

Krawczynski H, Muleri F, Dovčiak M, Veledina A, Rodriguez Cavero N, Svoboda J et al. Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1. Science. 2022;378(6620):650-654. https://doi.org/10.1126/science.add5399

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. In: Science. 2022 ; Vol. 378, No. 6620. pp. 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 -

ID: 104694373