Standard
Cygnus X-3 revealed as a Galactic ultraluminous X-ray source by IXPE. / Veledina, Alexandra; Muleri, Fabio; Poutanen, Juri; Podgorný, Jakub; Dovčiak, Michal; Capitanio, Fiamma; Churazov, Eugene; De Rosa, Alessandra; Di Marco, Alessandro; Forsblom, Sofia V.; Kaaret, Philip; Krawczynski, Henric; La Monaca, Fabio; Loktev, Vladislav; Lutovinov, Alexander A.; Molkov, Sergey V.; Mushtukov, Alexander A.; Ratheesh, Ajay; Rodriguez Cavero, Nicole; Steiner, James F.; Sunyaev, Rashid A.; Tsygankov, Sergey S.; Weisskopf, Martin C.; Zdziarski, Andrzej A.; Bianchi, Stefano; Bright, Joe S.; Bursov, Nikolaj; Costa, Enrico; Egron, Elise; Garcia, Javier A.; Green, David A.; Gurwell, Mark; Ingram, Adam; Kajava, Jari J. E.; Kale, Ruta; Kraus, Alex; Malyshev, Denys; Marin, Frédéric; Matt, Giorgio; McCollough, Michael; Mereminskiy, Ilya A.; Nizhelsky, Nikolaj; Piano, Giovanni; Pilia, Maura; Pittori, Carlotta; Rao, Ramprasad; Righini, Simona; Soffitta, Paolo; Shevchenko, Anton; Svoboda, Jiri; Tombesi, Francesco; Trushkin, Sergei A.; Tsybulev, Peter; Ursini, Francesco; Wu, Kinwah; 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; Chen, Chien-Ting; Ciprini, Stefano; Del Monte, Ettore; Di Gesu, Laura; Di Lalla, Niccolò; Donnarumma, Immacolata; Doroshenko, Victor; Ehlert, Steven R.; Enoto, Teruaki; Evangelista, Yuri; Fabiani, Sergio; Ferrazzoli, Riccardo; Gunji, Shuichi; Hayashida, Kiyoshi; Heyl, Jeremy; Iwakiri, Wataru; Jorstad, Svetlana G.; Karas, Vladimir; Kislat, Fabian; Kitaguchi, Takao; Kolodziejczak, Jeffery J.; Latronico, Luca; Liodakis, Ioannis; Maldera, Simone; Manfreda, Alberto; Marinucci, Andrea; Marscher, Alan P.; Marshall, Herman L.; Massaro, Francesco; Mitsuishi, Ikuyuki; Mizuno, Tsunefumi; Negro, Michela; Ng, Chi-Yung; O'Dell, Stephen L.; Omodei, Nicola; Oppedisano, Chiara; Papitto, Alessandro; Pavlov, George G.; Peirson, Abel L.; Perri, Matteo; Pesce-Rollins, Melissa; Petrucci, Pierre-Olivier; Possenti, Andrea; Puccetti, Simonetta; Ramsey, Brian D.; Rankin, John; Roberts, Oliver; Romani, Roger W.; Sgrò, Carmelo; Slane, Patrick; Spandre, Gloria; Swartz, Doug; Tamagawa, Toru; Tavecchio, Fabrizio; Taverna, Roberto; Tawara, Yuzuru; Tennant, Allyn F.; Thomas, Nicholas E.; Trois, Alessio; Turolla, Roberto; Vink, Jacco; Xie, Fei; Zane, Silvia.
в:
Nature Astronomy, 21.06.2024.
Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
Harvard
Veledina, A, Muleri, F, Poutanen, J, Podgorný, J, Dovčiak, M, Capitanio, F, Churazov, E, De Rosa, A, Di Marco, A, Forsblom, SV, Kaaret, P, Krawczynski, H, La Monaca, F
, Loktev, V, Lutovinov, AA, Molkov, SV, Mushtukov, AA, Ratheesh, A, Rodriguez Cavero, N, Steiner, JF, Sunyaev, RA, Tsygankov, SS, Weisskopf, MC, Zdziarski, AA, Bianchi, S, Bright, JS, Bursov, N, Costa, E, Egron, E, Garcia, JA, Green, DA, Gurwell, M, Ingram, A, Kajava, JJE, Kale, R, Kraus, A, Malyshev, D, Marin, F, Matt, G, McCollough, M, Mereminskiy, IA, Nizhelsky, N, Piano, G, Pilia, M, Pittori, C, Rao, R, Righini, S, Soffitta, P, Shevchenko, A, Svoboda, J, Tombesi, F, Trushkin, SA, Tsybulev, P, Ursini, F, Wu, K, Agudo, I, Antonelli, LA, Bachetti, M, Baldini, L, Baumgartner, WH, Bellazzini, R, Bongiorno, SD, Bonino, R, Brez, A, Bucciantini, N, Castellano, S, Cavazzuti, E, Chen, C-T, Ciprini, S, Del Monte, E, Di Gesu, L, Di Lalla, N, Donnarumma, I, Doroshenko, V, Ehlert, SR, Enoto, T, Evangelista, Y, Fabiani, S, Ferrazzoli, R, Gunji, S, Hayashida, K, Heyl, J, Iwakiri, W
, Jorstad, SG, Karas, V, Kislat, F, Kitaguchi, T, Kolodziejczak, JJ, Latronico, L, Liodakis, I, Maldera, S, Manfreda, A, Marinucci, A, Marscher, AP, Marshall, HL, Massaro, F, Mitsuishi, I, Mizuno, T, Negro, M, Ng, C-Y, O'Dell, SL, Omodei, N, Oppedisano, C, Papitto, A, Pavlov, GG, Peirson, AL, Perri, M, Pesce-Rollins, M, Petrucci, P-O, Possenti, A, Puccetti, S, Ramsey, BD, Rankin, J, Roberts, O, Romani, RW, Sgrò, C, Slane, P, Spandre, G, Swartz, D, Tamagawa, T, Tavecchio, F, Taverna, R, Tawara, Y, Tennant, AF, Thomas, NE, Trois, A, Turolla, R, Vink, J, Xie, F & Zane, S 2024, '
Cygnus X-3 revealed as a Galactic ultraluminous X-ray source by IXPE',
Nature Astronomy.
https://doi.org/10.1038/s41550-024-02294-9APA
Veledina, A., Muleri, F., Poutanen, J., Podgorný, J., Dovčiak, M., Capitanio, F., Churazov, E., De Rosa, A., Di Marco, A., Forsblom, S. V., Kaaret, P., Krawczynski, H., La Monaca, F.
, Loktev, V., Lutovinov, A. A., Molkov, S. V., Mushtukov, A. A., Ratheesh, A., Rodriguez Cavero, N., ... Zane, S. (2024).
Cygnus X-3 revealed as a Galactic ultraluminous X-ray source by IXPE.
Nature Astronomy.
https://doi.org/10.1038/s41550-024-02294-9Vancouver
Author
Veledina, Alexandra ; Muleri, Fabio ; Poutanen, Juri ; Podgorný, Jakub ; Dovčiak, Michal ; Capitanio, Fiamma ; Churazov, Eugene ; De Rosa, Alessandra ; Di Marco, Alessandro ; Forsblom, Sofia V. ; Kaaret, Philip ; Krawczynski, Henric ; La Monaca, Fabio
; Loktev, Vladislav ; Lutovinov, Alexander A. ; Molkov, Sergey V. ; Mushtukov, Alexander A. ; Ratheesh, Ajay ; Rodriguez Cavero, Nicole ; Steiner, James F. ; Sunyaev, Rashid A. ; Tsygankov, Sergey S. ; Weisskopf, Martin C. ; Zdziarski, Andrzej A. ; Bianchi, Stefano ; Bright, Joe S. ; Bursov, Nikolaj ; Costa, Enrico ; Egron, Elise ; Garcia, Javier A. ; Green, David A. ; Gurwell, Mark ; Ingram, Adam ; Kajava, Jari J. E. ; Kale, Ruta ; Kraus, Alex ; Malyshev, Denys ; Marin, Frédéric ; Matt, Giorgio ; McCollough, Michael ; Mereminskiy, Ilya A. ; Nizhelsky, Nikolaj ; Piano, Giovanni ; Pilia, Maura ; Pittori, Carlotta ; Rao, Ramprasad ; Righini, Simona ; Soffitta, Paolo ; Shevchenko, Anton ; Svoboda, Jiri ; Tombesi, Francesco ; Trushkin, Sergei A. ; Tsybulev, Peter ; Ursini, Francesco ; Wu, Kinwah ; 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 ; Chen, Chien-Ting ; Ciprini, Stefano ; Del Monte, Ettore ; Di Gesu, Laura ; Di Lalla, Niccolò ; Donnarumma, Immacolata ; Doroshenko, Victor ; Ehlert, Steven R. ; Enoto, Teruaki ; Evangelista, Yuri ; Fabiani, Sergio ; Ferrazzoli, Riccardo ; Gunji, Shuichi ; Hayashida, Kiyoshi ; Heyl, Jeremy ; Iwakiri, Wataru
; Jorstad, Svetlana G. ; Karas, Vladimir ; Kislat, Fabian ; Kitaguchi, Takao ; Kolodziejczak, Jeffery J. ; Latronico, Luca ; Liodakis, Ioannis ; Maldera, Simone ; Manfreda, Alberto ; Marinucci, Andrea ; Marscher, Alan P. ; Marshall, Herman L. ; Massaro, Francesco ; Mitsuishi, Ikuyuki ; Mizuno, Tsunefumi ; Negro, Michela ; Ng, Chi-Yung ; O'Dell, Stephen L. ; Omodei, Nicola ; Oppedisano, Chiara ; Papitto, Alessandro ; Pavlov, George G. ; Peirson, Abel L. ; Perri, Matteo ; Pesce-Rollins, Melissa ; Petrucci, Pierre-Olivier ; Possenti, Andrea ; Puccetti, Simonetta ; Ramsey, Brian D. ; Rankin, John ; Roberts, Oliver ; Romani, Roger W. ; Sgrò, Carmelo ; Slane, Patrick ; Spandre, Gloria ; Swartz, Doug ; Tamagawa, Toru ; Tavecchio, Fabrizio ; Taverna, Roberto ; Tawara, Yuzuru ; Tennant, Allyn F. ; Thomas, Nicholas E. ; Trois, Alessio ; Turolla, Roberto ; Vink, Jacco ; Xie, Fei ; Zane, Silvia. /
Cygnus X-3 revealed as a Galactic ultraluminous X-ray source by IXPE. в:
Nature Astronomy. 2024.
BibTeX
@article{dd40f6e00a214b47a5f402feea518823,
title = "Cygnus X-3 revealed as a Galactic ultraluminous X-ray source by IXPE",
abstract = "The accretion of matter by compact objects can be inhibited by radiation pressure if the luminosity exceeds a critical value known as the Eddington limit. The discovery of ultraluminous X-ray sources has shown that accretion can proceed even when the apparent luminosity considerably exceeds this limit. A high apparent luminosity might be produced due to the geometric beaming of radiation by an outflow. The outflow half-opening angle, which determines the amplification due to beaming, has never been robustly constrained. Using the Imaging X-ray Polarimetry Explorer, we measured the X-ray polarization in the Galactic X-ray binary Cygnus X-3 (Cyg X-3). We found high, >20%, nearly energy-independent linear polarization orthogonal to the direction of the radio ejections. These properties unambiguously indicate the presence of a collimating outflow from the X-ray binary Cyg X-3 and constrain its half-opening angle to ≲15°. Thus, the source can be used as a laboratory for studying the supercritical accretion regime. This finding underscores the importance of X-ray polarimetry in advancing our understanding of accreting sources.",
author = "Alexandra Veledina and Fabio Muleri and Juri Poutanen and Jakub Podgorn{\'y} and Michal Dov{\v c}iak and Fiamma Capitanio and Eugene Churazov and {De Rosa}, Alessandra and {Di Marco}, Alessandro and Forsblom, {Sofia V.} and Philip Kaaret and Henric Krawczynski and {La Monaca}, Fabio and Vladislav Loktev and Lutovinov, {Alexander A.} and Molkov, {Sergey V.} and Mushtukov, {Alexander A.} and Ajay Ratheesh and {Rodriguez Cavero}, Nicole and Steiner, {James F.} and Sunyaev, {Rashid A.} and Tsygankov, {Sergey S.} and Weisskopf, {Martin C.} and Zdziarski, {Andrzej A.} and Stefano Bianchi and Bright, {Joe S.} and Nikolaj Bursov and Enrico Costa and Elise Egron and Garcia, {Javier A.} and Green, {David A.} and Mark Gurwell and Adam Ingram and Kajava, {Jari J. E.} and Ruta Kale and Alex Kraus and Denys Malyshev and Fr{\'e}d{\'e}ric Marin and Giorgio Matt and Michael McCollough and Mereminskiy, {Ilya A.} and Nikolaj Nizhelsky and Giovanni Piano and Maura Pilia and Carlotta Pittori and Ramprasad Rao and Simona Righini and Paolo Soffitta and Anton Shevchenko and Jiri Svoboda and Francesco Tombesi and Trushkin, {Sergei A.} and Peter Tsybulev and Francesco Ursini and Kinwah Wu 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 Chien-Ting Chen and Stefano Ciprini and {Del Monte}, Ettore and {Di Gesu}, Laura and {Di Lalla}, Niccol{\`o} and Immacolata Donnarumma and Victor Doroshenko and Ehlert, {Steven R.} and Teruaki Enoto and Yuri Evangelista and Sergio Fabiani and Riccardo Ferrazzoli and Shuichi Gunji and Kiyoshi Hayashida and Jeremy Heyl and Wataru Iwakiri and Jorstad, {Svetlana G.} and Vladimir Karas and Fabian Kislat and Takao Kitaguchi and Kolodziejczak, {Jeffery J.} and Luca Latronico and Ioannis Liodakis and Simone Maldera and Alberto Manfreda and Andrea Marinucci and Marscher, {Alan P.} and Marshall, {Herman L.} and Francesco Massaro and Ikuyuki Mitsuishi and Tsunefumi Mizuno and Michela Negro and Chi-Yung Ng and O'Dell, {Stephen L.} and Nicola Omodei and Chiara Oppedisano and Alessandro Papitto and Pavlov, {George G.} and Peirson, {Abel L.} and Matteo Perri and Melissa Pesce-Rollins and Pierre-Olivier Petrucci and Andrea Possenti and Simonetta Puccetti and Ramsey, {Brian D.} and John Rankin and Oliver Roberts and Romani, {Roger W.} and Carmelo Sgr{\`o} and Patrick Slane and Gloria Spandre and Doug Swartz and Toru Tamagawa and Fabrizio Tavecchio and Roberto Taverna and Yuzuru Tawara and Tennant, {Allyn F.} and Thomas, {Nicholas E.} and Alessio Trois and Roberto Turolla and Jacco Vink and Fei Xie and Silvia Zane",
year = "2024",
month = jun,
day = "21",
doi = "10.1038/s41550-024-02294-9",
language = "русский",
journal = "Nature Astronomy",
issn = "2397-3366",
publisher = "Nature Publishing Group",
}
RIS
TY - JOUR
T1 - Cygnus X-3 revealed as a Galactic ultraluminous X-ray source by IXPE
AU - Veledina, Alexandra
AU - Muleri, Fabio
AU - Poutanen, Juri
AU - Podgorný, Jakub
AU - Dovčiak, Michal
AU - Capitanio, Fiamma
AU - Churazov, Eugene
AU - De Rosa, Alessandra
AU - Di Marco, Alessandro
AU - Forsblom, Sofia V.
AU - Kaaret, Philip
AU - Krawczynski, Henric
AU - La Monaca, Fabio
AU - Loktev, Vladislav
AU - Lutovinov, Alexander A.
AU - Molkov, Sergey V.
AU - Mushtukov, Alexander A.
AU - Ratheesh, Ajay
AU - Rodriguez Cavero, Nicole
AU - Steiner, James F.
AU - Sunyaev, Rashid A.
AU - Tsygankov, Sergey S.
AU - Weisskopf, Martin C.
AU - Zdziarski, Andrzej A.
AU - Bianchi, Stefano
AU - Bright, Joe S.
AU - Bursov, Nikolaj
AU - Costa, Enrico
AU - Egron, Elise
AU - Garcia, Javier A.
AU - Green, David A.
AU - Gurwell, Mark
AU - Ingram, Adam
AU - Kajava, Jari J. E.
AU - Kale, Ruta
AU - Kraus, Alex
AU - Malyshev, Denys
AU - Marin, Frédéric
AU - Matt, Giorgio
AU - McCollough, Michael
AU - Mereminskiy, Ilya A.
AU - Nizhelsky, Nikolaj
AU - Piano, Giovanni
AU - Pilia, Maura
AU - Pittori, Carlotta
AU - Rao, Ramprasad
AU - Righini, Simona
AU - Soffitta, Paolo
AU - Shevchenko, Anton
AU - Svoboda, Jiri
AU - Tombesi, Francesco
AU - Trushkin, Sergei A.
AU - Tsybulev, Peter
AU - Ursini, Francesco
AU - Wu, Kinwah
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 - Chen, Chien-Ting
AU - Ciprini, Stefano
AU - Del Monte, Ettore
AU - Di Gesu, Laura
AU - Di Lalla, Niccolò
AU - Donnarumma, Immacolata
AU - Doroshenko, Victor
AU - Ehlert, Steven R.
AU - Enoto, Teruaki
AU - Evangelista, Yuri
AU - Fabiani, Sergio
AU - Ferrazzoli, Riccardo
AU - Gunji, Shuichi
AU - Hayashida, Kiyoshi
AU - Heyl, Jeremy
AU - Iwakiri, Wataru
AU - Jorstad, Svetlana G.
AU - Karas, Vladimir
AU - Kislat, Fabian
AU - Kitaguchi, Takao
AU - Kolodziejczak, Jeffery J.
AU - Latronico, Luca
AU - Liodakis, Ioannis
AU - Maldera, Simone
AU - Manfreda, Alberto
AU - Marinucci, Andrea
AU - Marscher, Alan P.
AU - Marshall, Herman L.
AU - Massaro, Francesco
AU - Mitsuishi, Ikuyuki
AU - Mizuno, Tsunefumi
AU - Negro, Michela
AU - Ng, Chi-Yung
AU - O'Dell, Stephen L.
AU - Omodei, Nicola
AU - Oppedisano, Chiara
AU - Papitto, Alessandro
AU - Pavlov, George G.
AU - Peirson, Abel L.
AU - Perri, Matteo
AU - Pesce-Rollins, Melissa
AU - Petrucci, Pierre-Olivier
AU - Possenti, Andrea
AU - Puccetti, Simonetta
AU - Ramsey, Brian D.
AU - Rankin, John
AU - Roberts, Oliver
AU - Romani, Roger W.
AU - Sgrò, Carmelo
AU - Slane, Patrick
AU - Spandre, Gloria
AU - Swartz, Doug
AU - Tamagawa, Toru
AU - Tavecchio, Fabrizio
AU - Taverna, Roberto
AU - Tawara, Yuzuru
AU - Tennant, Allyn F.
AU - Thomas, Nicholas E.
AU - Trois, Alessio
AU - Turolla, Roberto
AU - Vink, Jacco
AU - Xie, Fei
AU - Zane, Silvia
PY - 2024/6/21
Y1 - 2024/6/21
N2 - The accretion of matter by compact objects can be inhibited by radiation pressure if the luminosity exceeds a critical value known as the Eddington limit. The discovery of ultraluminous X-ray sources has shown that accretion can proceed even when the apparent luminosity considerably exceeds this limit. A high apparent luminosity might be produced due to the geometric beaming of radiation by an outflow. The outflow half-opening angle, which determines the amplification due to beaming, has never been robustly constrained. Using the Imaging X-ray Polarimetry Explorer, we measured the X-ray polarization in the Galactic X-ray binary Cygnus X-3 (Cyg X-3). We found high, >20%, nearly energy-independent linear polarization orthogonal to the direction of the radio ejections. These properties unambiguously indicate the presence of a collimating outflow from the X-ray binary Cyg X-3 and constrain its half-opening angle to ≲15°. Thus, the source can be used as a laboratory for studying the supercritical accretion regime. This finding underscores the importance of X-ray polarimetry in advancing our understanding of accreting sources.
AB - The accretion of matter by compact objects can be inhibited by radiation pressure if the luminosity exceeds a critical value known as the Eddington limit. The discovery of ultraluminous X-ray sources has shown that accretion can proceed even when the apparent luminosity considerably exceeds this limit. A high apparent luminosity might be produced due to the geometric beaming of radiation by an outflow. The outflow half-opening angle, which determines the amplification due to beaming, has never been robustly constrained. Using the Imaging X-ray Polarimetry Explorer, we measured the X-ray polarization in the Galactic X-ray binary Cygnus X-3 (Cyg X-3). We found high, >20%, nearly energy-independent linear polarization orthogonal to the direction of the radio ejections. These properties unambiguously indicate the presence of a collimating outflow from the X-ray binary Cyg X-3 and constrain its half-opening angle to ≲15°. Thus, the source can be used as a laboratory for studying the supercritical accretion regime. This finding underscores the importance of X-ray polarimetry in advancing our understanding of accreting sources.
UR - https://www.mendeley.com/catalogue/5db89f3c-6626-305f-9a62-c1d8b55c16b4/
U2 - 10.1038/s41550-024-02294-9
DO - 10.1038/s41550-024-02294-9
M3 - статья
JO - Nature Astronomy
JF - Nature Astronomy
SN - 2397-3366
ER -
