Standard
Pulsar-wind-nebula-powered Galactic center X-ray filament G0.13-0.11. Proof of the synchrotron nature by IXPE. / Churazov, Eugene; Khabibullin, Ildar; Barnouin, Thibault; Bucciantini, Niccolò; Costa, Enrico; Di Gesu, Laura; Di Marco, Alessandro; Ferrazzoli, Riccardo; Forman, William; Kaaret, Philip; Kim, Dawoon E.; Kolodziejczak, Jeffery J.; Kraft, Ralph; Marin, Frédéric; Matt, Giorgio; Negro, Michela; Romani, Roger W.; Silvestri, Stefano; Soffitta, Paolo; Sunyaev, Rashid; Svoboda, Jiri; Vikhlinin, Alexey; Weisskopf, Martin C.; Xie, Fei; Agudo, Iván; Antonelli, Lucio A.; Bachetti, Matteo; Baldini, Luca; Baumgartner, Wayne H.; Bellazzini, Ronaldo; Bianchi, Stefano; Bongiorno, Stephen D.; Bonino, Raffaella; Brez, Alessandro; Capitanio, Fiamma; Castellano, Simone; Cavazzuti, Elisabetta; Chen, Chien-Ting; Ciprini, Stefano; De Rosa, Alessandra; Del Monte, Ettore; Di Lalla, Niccolò; Donnarumma, Immacolata; Doroshenko, Victor; Dovčiak, Michal; Ehlert, Steven R.; Enoto, Teruaki; Evangelista, Yuri; Fabiani, Sergio; García, Javier A.; Gunji, Shuichi; Hayashida, Kiyoshi; Heyl, Jeremy; Iwakiri, Wataru; Jorstad, Svetlana G.; Karas, Vladimir; Kislat, Fabian; Kitaguchi, Takao; Krawczynski, Henric; La Monaca, Fabio; Latronico, Luca; Liodakis, Ioannis; Maldera, Simone; Manfreda, Alberto; Marinucci, Andrea; Marscher, Alan P.; Marshall, Herman L.; Massaro, Francesco; Mitsuishi, Ikuyuki; Mizuno, Tsunefumi; Muleri, Fabio; 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; Pilia, Maura; Possenti, Andrea; Poutanen, Juri; Puccetti, Simonetta; Ramsey, Brian D.; Rankin, John; Ratheesh, Ajay; Roberts, Oliver J.; Sgrò, Carmelo; Slane, Patrick; Spandre, Gloria; Swartz, Douglas A.; Tamagawa, Toru; Tavecchio, Fabrizio; Taverna, Roberto; Tawara, Yuzuru; Tennant, Allyn F.; Thomas, Nicholas E.; Tombesi, Francesco; Trois, Alessio; Tsygankov, Sergey S.; Turolla, Roberto; Vink, Jacco; Wu, Kinwah; Zane, Silvia.
In:
Astronomy and Astrophysics, Vol. 686, 24.05.2024, p. A14.
Research output: Contribution to journal › Article › peer-review
Harvard
Churazov, E, Khabibullin, I, Barnouin, T, Bucciantini, N, Costa, E, Di Gesu, L, Di Marco, A, Ferrazzoli, R, Forman, W, Kaaret, P, Kim, DE, Kolodziejczak, JJ, Kraft, R, Marin, F, Matt, G, Negro, M, Romani, RW, Silvestri, S, Soffitta, P, Sunyaev, R, Svoboda, J, Vikhlinin, A, Weisskopf, MC, Xie, F, Agudo, I, Antonelli, LA, Bachetti, M, Baldini, L, Baumgartner, WH, Bellazzini, R, Bianchi, S, Bongiorno, SD, Bonino, R, Brez, A, Capitanio, F, Castellano, S, Cavazzuti, E, Chen, C-T, Ciprini, S, De Rosa, A, Del Monte, E, Di Lalla, N, Donnarumma, I, Doroshenko, V, Dovčiak, M, Ehlert, SR, Enoto, T, Evangelista, Y, Fabiani, S, García, JA, Gunji, S, Hayashida, K, Heyl, J, Iwakiri, W
, Jorstad, SG, Karas, V, Kislat, F, Kitaguchi, T, Krawczynski, H, La Monaca, F, Latronico, L, Liodakis, I, Maldera, S, Manfreda, A, Marinucci, A, Marscher, AP, Marshall, HL, Massaro, F, Mitsuishi, I, Mizuno, T, Muleri, F, Ng, C-Y, O'Dell, SL, Omodei, N, Oppedisano, C, Papitto, A, Pavlov, GG, Peirson, AL, Perri, M, Pesce-Rollins, M, Petrucci, P-O, Pilia, M, Possenti, A, Poutanen, J, Puccetti, S, Ramsey, BD, Rankin, J, Ratheesh, A, Roberts, OJ, Sgrò, C, Slane, P, Spandre, G, Swartz, DA, Tamagawa, T, Tavecchio, F, Taverna, R, Tawara, Y, Tennant, AF, Thomas, NE, Tombesi, F, Trois, A, Tsygankov, SS, Turolla, R, Vink, J, Wu, K & Zane, S 2024, '
Pulsar-wind-nebula-powered Galactic center X-ray filament G0.13-0.11. Proof of the synchrotron nature by IXPE',
Astronomy and Astrophysics, vol. 686, pp. A14.
https://doi.org/10.1051/0004-6361/202349080APA
Churazov, E., Khabibullin, I., Barnouin, T., Bucciantini, N., Costa, E., Di Gesu, L., Di Marco, A., Ferrazzoli, R., Forman, W., Kaaret, P., Kim, D. E., Kolodziejczak, J. J., Kraft, R., Marin, F., Matt, G., Negro, M., Romani, R. W., Silvestri, S., Soffitta, P., ... Zane, S. (2024).
Pulsar-wind-nebula-powered Galactic center X-ray filament G0.13-0.11. Proof of the synchrotron nature by IXPE.
Astronomy and Astrophysics,
686, A14.
https://doi.org/10.1051/0004-6361/202349080Vancouver
Author
Churazov, Eugene ; Khabibullin, Ildar ; Barnouin, Thibault ; Bucciantini, Niccolò ; Costa, Enrico ; Di Gesu, Laura ; Di Marco, Alessandro ; Ferrazzoli, Riccardo ; Forman, William ; Kaaret, Philip ; Kim, Dawoon E. ; Kolodziejczak, Jeffery J. ; Kraft, Ralph ; Marin, Frédéric ; Matt, Giorgio ; Negro, Michela ; Romani, Roger W. ; Silvestri, Stefano ; Soffitta, Paolo ; Sunyaev, Rashid ; Svoboda, Jiri ; Vikhlinin, Alexey ; Weisskopf, Martin C. ; Xie, Fei ; Agudo, Iván ; Antonelli, Lucio A. ; Bachetti, Matteo ; Baldini, Luca ; Baumgartner, Wayne H. ; Bellazzini, Ronaldo ; Bianchi, Stefano ; Bongiorno, Stephen D. ; Bonino, Raffaella ; Brez, Alessandro ; Capitanio, Fiamma ; Castellano, Simone ; Cavazzuti, Elisabetta ; Chen, Chien-Ting ; Ciprini, Stefano ; De Rosa, Alessandra ; Del Monte, Ettore ; Di Lalla, Niccolò ; Donnarumma, Immacolata ; Doroshenko, Victor ; Dovčiak, Michal ; Ehlert, Steven R. ; Enoto, Teruaki ; Evangelista, Yuri ; Fabiani, Sergio ; García, Javier A. ; Gunji, Shuichi ; Hayashida, Kiyoshi ; Heyl, Jeremy ; Iwakiri, Wataru
; Jorstad, Svetlana G. ; Karas, Vladimir ; Kislat, Fabian ; Kitaguchi, Takao ; Krawczynski, Henric ; La Monaca, Fabio ; Latronico, Luca ; Liodakis, Ioannis ; Maldera, Simone ; Manfreda, Alberto ; Marinucci, Andrea ; Marscher, Alan P. ; Marshall, Herman L. ; Massaro, Francesco ; Mitsuishi, Ikuyuki ; Mizuno, Tsunefumi ; Muleri, Fabio ; 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 ; Pilia, Maura ; Possenti, Andrea ; Poutanen, Juri ; Puccetti, Simonetta ; Ramsey, Brian D. ; Rankin, John ; Ratheesh, Ajay ; Roberts, Oliver J. ; Sgrò, Carmelo ; Slane, Patrick ; Spandre, Gloria ; Swartz, Douglas A. ; Tamagawa, Toru ; Tavecchio, Fabrizio ; Taverna, Roberto ; Tawara, Yuzuru ; Tennant, Allyn F. ; Thomas, Nicholas E. ; Tombesi, Francesco ; Trois, Alessio ; Tsygankov, Sergey S. ; Turolla, Roberto ; Vink, Jacco ; Wu, Kinwah ; Zane, Silvia. /
Pulsar-wind-nebula-powered Galactic center X-ray filament G0.13-0.11. Proof of the synchrotron nature by IXPE. In:
Astronomy and Astrophysics. 2024 ; Vol. 686. pp. A14.
BibTeX
@article{3218ec57176846a0ab830999000bb162,
title = "Pulsar-wind-nebula-powered Galactic center X-ray filament G0.13-0.11. Proof of the synchrotron nature by IXPE",
abstract = "We report the discovery of X-ray polarization from the X-ray-bright filament G0.13−0.11 in the Galactic center (GC) region. This filament features a bright, hard X-ray source that is most plausibly a pulsar wind nebula (PWN) and an extended and structured diffuse component. Combining the polarization signal from IXPE with the imaging/spectroscopic data from Chandra, we find that X-ray emission of G0.13−0.11 is highly polarized PD = 57(±18)% in the 3−6 keV band, while the polarization angle is PA = 21 ° ( ± 9 °). This high degree of polarization proves the synchrotron origin of the X-ray emission from G0.13−0.11. In turn, the measured polarization angle implies that the X-ray emission is polarized approximately perpendicular to a sequence of nonthermal radio filaments that may be part of the GC Radio Arc. The magnetic field on the order of 100 μG appears to be preferentially ordered along the filaments. The above field strength is the fiducial value that makes our model self-consistent, while the other conclusions are largely model independent.",
keywords = "magnetic fields, polarization, radiation mechanisms: non-thermal, scattering, X-rays: general, Astrophysics - High Energy Astrophysical Phenomena, Magnetic fields, Polarization, Radiation mechanisms: non-thermal, Scattering, X-rays: general",
author = "Eugene Churazov and Ildar Khabibullin and Thibault Barnouin and Niccol{\`o} Bucciantini and Enrico Costa and {Di Gesu}, Laura and {Di Marco}, Alessandro and Riccardo Ferrazzoli and William Forman and Philip Kaaret and Kim, {Dawoon E.} and Kolodziejczak, {Jeffery J.} and Ralph Kraft and Fr{\'e}d{\'e}ric Marin and Giorgio Matt and Michela Negro and Romani, {Roger W.} and Stefano Silvestri and Paolo Soffitta and Rashid Sunyaev and Jiri Svoboda and Alexey Vikhlinin and Weisskopf, {Martin C.} and Fei Xie and Iv{\'a}n Agudo and Antonelli, {Lucio A.} and Matteo Bachetti and Luca Baldini and Baumgartner, {Wayne H.} and Ronaldo Bellazzini and Stefano Bianchi and Bongiorno, {Stephen D.} and Raffaella Bonino and Alessandro Brez and Fiamma Capitanio and Simone Castellano and Elisabetta Cavazzuti and Chien-Ting Chen and Stefano Ciprini and {De Rosa}, Alessandra and {Del Monte}, Ettore and {Di Lalla}, Niccol{\`o} and Immacolata Donnarumma and Victor Doroshenko and Michal Dov{\v c}iak and Ehlert, {Steven R.} and Teruaki Enoto and Yuri Evangelista and Sergio Fabiani and Garc{\'i}a, {Javier A.} 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 Henric Krawczynski and {La Monaca}, Fabio 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 Fabio Muleri 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 Maura Pilia and Andrea Possenti and Juri Poutanen and Simonetta Puccetti and Ramsey, {Brian D.} and John Rankin and Ajay Ratheesh and Roberts, {Oliver J.} and Carmelo Sgr{\`o} and Patrick Slane and Gloria Spandre and Swartz, {Douglas A.} and Toru Tamagawa and Fabrizio Tavecchio and Roberto Taverna and Yuzuru Tawara and Tennant, {Allyn F.} and Thomas, {Nicholas E.} and Francesco Tombesi and Alessio Trois and Tsygankov, {Sergey S.} and Roberto Turolla and Jacco Vink and Kinwah Wu and Silvia Zane",
year = "2024",
month = may,
day = "24",
doi = "10.1051/0004-6361/202349080",
language = "русский",
volume = "686",
pages = "A14",
journal = "ASTRONOMY & ASTROPHYSICS",
issn = "0004-6361",
publisher = "EDP Sciences",
}
RIS
TY - JOUR
T1 - Pulsar-wind-nebula-powered Galactic center X-ray filament G0.13-0.11. Proof of the synchrotron nature by IXPE
AU - Churazov, Eugene
AU - Khabibullin, Ildar
AU - Barnouin, Thibault
AU - Bucciantini, Niccolò
AU - Costa, Enrico
AU - Di Gesu, Laura
AU - Di Marco, Alessandro
AU - Ferrazzoli, Riccardo
AU - Forman, William
AU - Kaaret, Philip
AU - Kim, Dawoon E.
AU - Kolodziejczak, Jeffery J.
AU - Kraft, Ralph
AU - Marin, Frédéric
AU - Matt, Giorgio
AU - Negro, Michela
AU - Romani, Roger W.
AU - Silvestri, Stefano
AU - Soffitta, Paolo
AU - Sunyaev, Rashid
AU - Svoboda, Jiri
AU - Vikhlinin, Alexey
AU - Weisskopf, Martin C.
AU - Xie, Fei
AU - Agudo, Iván
AU - Antonelli, Lucio A.
AU - Bachetti, Matteo
AU - Baldini, Luca
AU - Baumgartner, Wayne H.
AU - Bellazzini, Ronaldo
AU - Bianchi, Stefano
AU - Bongiorno, Stephen D.
AU - Bonino, Raffaella
AU - Brez, Alessandro
AU - Capitanio, Fiamma
AU - Castellano, Simone
AU - Cavazzuti, Elisabetta
AU - Chen, Chien-Ting
AU - Ciprini, Stefano
AU - De Rosa, Alessandra
AU - Del Monte, Ettore
AU - Di Lalla, Niccolò
AU - Donnarumma, Immacolata
AU - Doroshenko, Victor
AU - Dovčiak, Michal
AU - Ehlert, Steven R.
AU - Enoto, Teruaki
AU - Evangelista, Yuri
AU - Fabiani, Sergio
AU - García, Javier A.
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 - Krawczynski, Henric
AU - La Monaca, Fabio
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 - Muleri, Fabio
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 - Pilia, Maura
AU - Possenti, Andrea
AU - Poutanen, Juri
AU - Puccetti, Simonetta
AU - Ramsey, Brian D.
AU - Rankin, John
AU - Ratheesh, Ajay
AU - Roberts, Oliver J.
AU - Sgrò, Carmelo
AU - Slane, Patrick
AU - Spandre, Gloria
AU - Swartz, Douglas A.
AU - Tamagawa, Toru
AU - Tavecchio, Fabrizio
AU - Taverna, Roberto
AU - Tawara, Yuzuru
AU - Tennant, Allyn F.
AU - Thomas, Nicholas E.
AU - Tombesi, Francesco
AU - Trois, Alessio
AU - Tsygankov, Sergey S.
AU - Turolla, Roberto
AU - Vink, Jacco
AU - Wu, Kinwah
AU - Zane, Silvia
PY - 2024/5/24
Y1 - 2024/5/24
N2 - We report the discovery of X-ray polarization from the X-ray-bright filament G0.13−0.11 in the Galactic center (GC) region. This filament features a bright, hard X-ray source that is most plausibly a pulsar wind nebula (PWN) and an extended and structured diffuse component. Combining the polarization signal from IXPE with the imaging/spectroscopic data from Chandra, we find that X-ray emission of G0.13−0.11 is highly polarized PD = 57(±18)% in the 3−6 keV band, while the polarization angle is PA = 21 ° ( ± 9 °). This high degree of polarization proves the synchrotron origin of the X-ray emission from G0.13−0.11. In turn, the measured polarization angle implies that the X-ray emission is polarized approximately perpendicular to a sequence of nonthermal radio filaments that may be part of the GC Radio Arc. The magnetic field on the order of 100 μG appears to be preferentially ordered along the filaments. The above field strength is the fiducial value that makes our model self-consistent, while the other conclusions are largely model independent.
AB - We report the discovery of X-ray polarization from the X-ray-bright filament G0.13−0.11 in the Galactic center (GC) region. This filament features a bright, hard X-ray source that is most plausibly a pulsar wind nebula (PWN) and an extended and structured diffuse component. Combining the polarization signal from IXPE with the imaging/spectroscopic data from Chandra, we find that X-ray emission of G0.13−0.11 is highly polarized PD = 57(±18)% in the 3−6 keV band, while the polarization angle is PA = 21 ° ( ± 9 °). This high degree of polarization proves the synchrotron origin of the X-ray emission from G0.13−0.11. In turn, the measured polarization angle implies that the X-ray emission is polarized approximately perpendicular to a sequence of nonthermal radio filaments that may be part of the GC Radio Arc. The magnetic field on the order of 100 μG appears to be preferentially ordered along the filaments. The above field strength is the fiducial value that makes our model self-consistent, while the other conclusions are largely model independent.
KW - magnetic fields
KW - polarization
KW - radiation mechanisms: non-thermal
KW - scattering
KW - X-rays: general
KW - Astrophysics - High Energy Astrophysical Phenomena
KW - Magnetic fields
KW - Polarization
KW - Radiation mechanisms: non-thermal
KW - Scattering
KW - X-rays: general
UR - https://www.mendeley.com/catalogue/d20bc645-6e39-33ac-bdcd-674b99a5fac1/
U2 - 10.1051/0004-6361/202349080
DO - 10.1051/0004-6361/202349080
M3 - статья
VL - 686
SP - A14
JO - ASTRONOMY & ASTROPHYSICS
JF - ASTRONOMY & ASTROPHYSICS
SN - 0004-6361
ER -
