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Discovery of a Shock-compressed Magnetic Field in the Northwestern Rim of the Young Supernova Remnant RX J1713.7–3946 with X-Ray Polarimetry. / Ferrazzoli, Riccardo; Prokhorov, Dmitry; Bucciantini, Niccolò; Slane, Patrick; Vink, Jacco; Cardillo, Martina; Yang, Yi-Jung; Silvestri, Stefano; Zhou, Ping; Costa, Enrico; Omodei, Nicola; Ng, C. -Y.; Soffitta, Paolo; Weisskopf, Martin C.; Baldini, Luca; Di Marco, Alessandro; Doroshenko, Victor; Heyl, Jeremy; Kaaret, Philip; Kim, Dawoon E.; Marin, Frédéric; Mizuno, Tsunefumi; Pesce-Rollins, Melissa; Sgrò, Carmelo; Swartz, Douglas A.; Tamagawa, Toru; Xie, Fei; Agudo, Iván; Antonelli, Lucio A.; Bachetti, Matteo; 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 Gesu, Laura; Di Lalla, Niccolò; Donnarumma, Immacolata; Dovčiak, Michal; Ehlert, Steven R.; Enoto, Teruaki; Evangelista, Yuri; Fabiani, Sergio; Garcia, Javier A.; Gunji, Shuichi; Hayashida, Kiyoshi; Iwakiri, Wataru; Jorstad, Svetlana G.; Karas, Vladimir; Kislat, Fabian; Kitaguchi, Takao; Kolodziejczak, Jeffery J.; Krawczynski, Henric; La Monaca, Fabio; Latronico, Luca; Liodakis, Ioannis; Maldera, Simone; Manfreda, Alberto; Marinucci, Andrea; Marscher, Alan P.; Marshall, Herman L.; Massaro, Francesco; Matt, Giorgio; Mitsuishi, Ikuyuki; Muleri, Fabio; Negro, Michela; O'Dell, Stephen L.; Oppedisano, Chiara; Papitto, Alessandro; Pavlov, George G.; Peirson, Abel L.; Perri, Matteo; Petrucci, Pierre-Olivier; Pilia, Maura; Possenti, Andrea; Poutanen, Juri; Puccetti, Simonetta; Ramsey, Brian D.; Rankin, John; Ratheesh, Ajay; Roberts, Oliver J.; Romani, Roger W.; Spandre, Gloria; Tavecchio, Fabrizio; Taverna, Roberto; Tawara, Yuzuru; Tennant, Allyn F.; Thomas, Nicholas E.; Tombesi, Francesco; Trois, Alessio; Tsygankov, Sergey S.; Turolla, Roberto; Wu, Kinwah; Zane, Silvia.

In: The Astrophysical Journal, Vol. 967, No. 2, 30.05.2024, p. L38.

Research output: Contribution to journalArticlepeer-review

Harvard

Ferrazzoli, R, Prokhorov, D, Bucciantini, N, Slane, P, Vink, J, Cardillo, M, Yang, Y-J, Silvestri, S, Zhou, P, Costa, E, Omodei, N, Ng, C-Y, Soffitta, P, Weisskopf, MC, Baldini, L, Di Marco, A, Doroshenko, V, Heyl, J, Kaaret, P, Kim, DE, Marin, F, Mizuno, T, Pesce-Rollins, M, Sgrò, C, Swartz, DA, Tamagawa, T, Xie, F, Agudo, I, Antonelli, LA, Bachetti, M, 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 Gesu, L, Di Lalla, N, Donnarumma, I, Dovčiak, M, Ehlert, SR, Enoto, T, Evangelista, Y, Fabiani, S, Garcia, JA, Gunji, S, Hayashida, K, Iwakiri, W, Jorstad, SG, Karas, V, Kislat, F, Kitaguchi, T, Kolodziejczak, JJ, Krawczynski, H, La Monaca, F, Latronico, L, Liodakis, I, Maldera, S, Manfreda, A, Marinucci, A, Marscher, AP, Marshall, HL, Massaro, F, Matt, G, Mitsuishi, I, Muleri, F, Negro, M, O'Dell, SL, Oppedisano, C, Papitto, A, Pavlov, GG, Peirson, AL, Perri, M, Petrucci, P-O, Pilia, M, Possenti, A, Poutanen, J, Puccetti, S, Ramsey, BD, Rankin, J, Ratheesh, A, Roberts, OJ, Romani, RW, Spandre, G, Tavecchio, F, Taverna, R, Tawara, Y, Tennant, AF, Thomas, NE, Tombesi, F, Trois, A, Tsygankov, SS, Turolla, R, Wu, K & Zane, S 2024, 'Discovery of a Shock-compressed Magnetic Field in the Northwestern Rim of the Young Supernova Remnant RX J1713.7–3946 with X-Ray Polarimetry', The Astrophysical Journal, vol. 967, no. 2, pp. L38. https://doi.org/10.3847/2041-8213/ad4a68

APA

Ferrazzoli, R., Prokhorov, D., Bucciantini, N., Slane, P., Vink, J., Cardillo, M., Yang, Y-J., Silvestri, S., Zhou, P., Costa, E., Omodei, N., Ng, C. -Y., Soffitta, P., Weisskopf, M. C., Baldini, L., Di Marco, A., Doroshenko, V., Heyl, J., Kaaret, P., ... Zane, S. (2024). Discovery of a Shock-compressed Magnetic Field in the Northwestern Rim of the Young Supernova Remnant RX J1713.7–3946 with X-Ray Polarimetry. The Astrophysical Journal, 967(2), L38. https://doi.org/10.3847/2041-8213/ad4a68

Vancouver

Ferrazzoli R, Prokhorov D, Bucciantini N, Slane P, Vink J, Cardillo M et al. Discovery of a Shock-compressed Magnetic Field in the Northwestern Rim of the Young Supernova Remnant RX J1713.7–3946 with X-Ray Polarimetry. The Astrophysical Journal. 2024 May 30;967(2):L38. https://doi.org/10.3847/2041-8213/ad4a68

Author

Ferrazzoli, Riccardo ; Prokhorov, Dmitry ; Bucciantini, Niccolò ; Slane, Patrick ; Vink, Jacco ; Cardillo, Martina ; Yang, Yi-Jung ; Silvestri, Stefano ; Zhou, Ping ; Costa, Enrico ; Omodei, Nicola ; Ng, C. -Y. ; Soffitta, Paolo ; Weisskopf, Martin C. ; Baldini, Luca ; Di Marco, Alessandro ; Doroshenko, Victor ; Heyl, Jeremy ; Kaaret, Philip ; Kim, Dawoon E. ; Marin, Frédéric ; Mizuno, Tsunefumi ; Pesce-Rollins, Melissa ; Sgrò, Carmelo ; Swartz, Douglas A. ; Tamagawa, Toru ; Xie, Fei ; Agudo, Iván ; Antonelli, Lucio A. ; Bachetti, Matteo ; 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 Gesu, Laura ; Di Lalla, Niccolò ; Donnarumma, Immacolata ; Dovčiak, Michal ; Ehlert, Steven R. ; Enoto, Teruaki ; Evangelista, Yuri ; Fabiani, Sergio ; Garcia, Javier A. ; Gunji, Shuichi ; Hayashida, Kiyoshi ; Iwakiri, Wataru ; Jorstad, Svetlana G. ; Karas, Vladimir ; Kislat, Fabian ; Kitaguchi, Takao ; Kolodziejczak, Jeffery J. ; Krawczynski, Henric ; La Monaca, Fabio ; Latronico, Luca ; Liodakis, Ioannis ; Maldera, Simone ; Manfreda, Alberto ; Marinucci, Andrea ; Marscher, Alan P. ; Marshall, Herman L. ; Massaro, Francesco ; Matt, Giorgio ; Mitsuishi, Ikuyuki ; Muleri, Fabio ; Negro, Michela ; O'Dell, Stephen L. ; Oppedisano, Chiara ; Papitto, Alessandro ; Pavlov, George G. ; Peirson, Abel L. ; Perri, Matteo ; Petrucci, Pierre-Olivier ; Pilia, Maura ; Possenti, Andrea ; Poutanen, Juri ; Puccetti, Simonetta ; Ramsey, Brian D. ; Rankin, John ; Ratheesh, Ajay ; Roberts, Oliver J. ; Romani, Roger W. ; Spandre, Gloria ; Tavecchio, Fabrizio ; Taverna, Roberto ; Tawara, Yuzuru ; Tennant, Allyn F. ; Thomas, Nicholas E. ; Tombesi, Francesco ; Trois, Alessio ; Tsygankov, Sergey S. ; Turolla, Roberto ; Wu, Kinwah ; Zane, Silvia. / Discovery of a Shock-compressed Magnetic Field in the Northwestern Rim of the Young Supernova Remnant RX J1713.7–3946 with X-Ray Polarimetry. In: The Astrophysical Journal. 2024 ; Vol. 967, No. 2. pp. L38.

BibTeX

@article{8b3856ed661c4909b3d6a55421025d9c,
title = "Discovery of a Shock-compressed Magnetic Field in the Northwestern Rim of the Young Supernova Remnant RX J1713.7–3946 with X-Ray Polarimetry",
abstract = "Supernova remnants (SNRs) provide insights into cosmic-ray acceleration and magnetic field dynamics at shock fronts. Recent X-ray polarimetric measurements by the Imaging X-ray Polarimetry Explorer (IXPE) have revealed radial magnetic fields near particle acceleration sites in young SNRs, including Cassiopeia A, Tycho, and SN 1006. We present here the spatially resolved IXPE X-ray polarimetric observation of the northwestern rim of SNR RX J1713.7–3946. For the first time, our analysis shows that the magnetic field in the particle acceleration sites of this SNR is oriented tangentially with respect to the shock front. Because of the lack of precise Faraday rotation measurements in the radio band, this was not possible before. The average measured polarization degree (PD) of the synchrotron emission is 12.5% ± 3.3%, lower than the one measured by IXPE in SN 1006, comparable to the Tycho one, but notably higher than the one in Cassiopeia A. On subparsec scales, localized patches within RX J1713.7–3946 display a PD of up to 41.5% ± 9.5%. These results are compatible with a shock-compressed magnetic field. However, in order to explain the observed PD, either the presence of a radial net magnetic field upstream of the shock or partial reisotropization of the turbulence downstream by radial magnetohydrodynamical instabilities can be invoked. From comparison of PD and magnetic field distribution with γ-rays and 12CO data, our results provide new inputs in favor of a leptonic origin of the γ-ray emission.",
keywords = "X-ray astronomy, Polarimetry, Supernova remnants, 1810, 1278, 1667, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies",
author = "Riccardo Ferrazzoli and Dmitry Prokhorov and Niccol{\`o} Bucciantini and Patrick Slane and Jacco Vink and Martina Cardillo and Yi-Jung Yang and Stefano Silvestri and Ping Zhou and Enrico Costa and Nicola Omodei and Ng, {C. -Y.} and Paolo Soffitta and Weisskopf, {Martin C.} and Luca Baldini and {Di Marco}, Alessandro and Victor Doroshenko and Jeremy Heyl and Philip Kaaret and Kim, {Dawoon E.} and Fr{\'e}d{\'e}ric Marin and Tsunefumi Mizuno and Melissa Pesce-Rollins and Carmelo Sgr{\`o} and Swartz, {Douglas A.} and Toru Tamagawa and Fei Xie and Iv{\'a}n Agudo and Antonelli, {Lucio A.} and Matteo Bachetti 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 Gesu}, Laura and {Di Lalla}, Niccol{\`o} and Immacolata Donnarumma and Michal Dov{\v c}iak and Ehlert, {Steven R.} and Teruaki Enoto and Yuri Evangelista and Sergio Fabiani and Garcia, {Javier A.} and Shuichi Gunji and Kiyoshi Hayashida and Wataru Iwakiri and Jorstad, {Svetlana G.} and Vladimir Karas and Fabian Kislat and Takao Kitaguchi and Kolodziejczak, {Jeffery J.} 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 Giorgio Matt and Ikuyuki Mitsuishi and Fabio Muleri and Michela Negro and O'Dell, {Stephen L.} and Chiara Oppedisano and Alessandro Papitto and Pavlov, {George G.} and Peirson, {Abel L.} and Matteo Perri 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 Romani, {Roger W.} and Gloria Spandre 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 Kinwah Wu and Silvia Zane",
year = "2024",
month = may,
day = "30",
doi = "10.3847/2041-8213/ad4a68",
language = "русский",
volume = "967",
pages = "L38",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "IOP Publishing Ltd.",
number = "2",

}

RIS

TY - JOUR

T1 - Discovery of a Shock-compressed Magnetic Field in the Northwestern Rim of the Young Supernova Remnant RX J1713.7–3946 with X-Ray Polarimetry

AU - Ferrazzoli, Riccardo

AU - Prokhorov, Dmitry

AU - Bucciantini, Niccolò

AU - Slane, Patrick

AU - Vink, Jacco

AU - Cardillo, Martina

AU - Yang, Yi-Jung

AU - Silvestri, Stefano

AU - Zhou, Ping

AU - Costa, Enrico

AU - Omodei, Nicola

AU - Ng, C. -Y.

AU - Soffitta, Paolo

AU - Weisskopf, Martin C.

AU - Baldini, Luca

AU - Di Marco, Alessandro

AU - Doroshenko, Victor

AU - Heyl, Jeremy

AU - Kaaret, Philip

AU - Kim, Dawoon E.

AU - Marin, Frédéric

AU - Mizuno, Tsunefumi

AU - Pesce-Rollins, Melissa

AU - Sgrò, Carmelo

AU - Swartz, Douglas A.

AU - Tamagawa, Toru

AU - Xie, Fei

AU - Agudo, Iván

AU - Antonelli, Lucio A.

AU - Bachetti, Matteo

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 Gesu, Laura

AU - Di Lalla, Niccolò

AU - Donnarumma, Immacolata

AU - Dovčiak, Michal

AU - Ehlert, Steven R.

AU - Enoto, Teruaki

AU - Evangelista, Yuri

AU - Fabiani, Sergio

AU - Garcia, Javier A.

AU - Gunji, Shuichi

AU - Hayashida, Kiyoshi

AU - Iwakiri, Wataru

AU - Jorstad, Svetlana G.

AU - Karas, Vladimir

AU - Kislat, Fabian

AU - Kitaguchi, Takao

AU - Kolodziejczak, Jeffery J.

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 - Matt, Giorgio

AU - Mitsuishi, Ikuyuki

AU - Muleri, Fabio

AU - Negro, Michela

AU - O'Dell, Stephen L.

AU - Oppedisano, Chiara

AU - Papitto, Alessandro

AU - Pavlov, George G.

AU - Peirson, Abel L.

AU - Perri, Matteo

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 - Romani, Roger W.

AU - Spandre, Gloria

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 - Wu, Kinwah

AU - Zane, Silvia

PY - 2024/5/30

Y1 - 2024/5/30

N2 - Supernova remnants (SNRs) provide insights into cosmic-ray acceleration and magnetic field dynamics at shock fronts. Recent X-ray polarimetric measurements by the Imaging X-ray Polarimetry Explorer (IXPE) have revealed radial magnetic fields near particle acceleration sites in young SNRs, including Cassiopeia A, Tycho, and SN 1006. We present here the spatially resolved IXPE X-ray polarimetric observation of the northwestern rim of SNR RX J1713.7–3946. For the first time, our analysis shows that the magnetic field in the particle acceleration sites of this SNR is oriented tangentially with respect to the shock front. Because of the lack of precise Faraday rotation measurements in the radio band, this was not possible before. The average measured polarization degree (PD) of the synchrotron emission is 12.5% ± 3.3%, lower than the one measured by IXPE in SN 1006, comparable to the Tycho one, but notably higher than the one in Cassiopeia A. On subparsec scales, localized patches within RX J1713.7–3946 display a PD of up to 41.5% ± 9.5%. These results are compatible with a shock-compressed magnetic field. However, in order to explain the observed PD, either the presence of a radial net magnetic field upstream of the shock or partial reisotropization of the turbulence downstream by radial magnetohydrodynamical instabilities can be invoked. From comparison of PD and magnetic field distribution with γ-rays and 12CO data, our results provide new inputs in favor of a leptonic origin of the γ-ray emission.

AB - Supernova remnants (SNRs) provide insights into cosmic-ray acceleration and magnetic field dynamics at shock fronts. Recent X-ray polarimetric measurements by the Imaging X-ray Polarimetry Explorer (IXPE) have revealed radial magnetic fields near particle acceleration sites in young SNRs, including Cassiopeia A, Tycho, and SN 1006. We present here the spatially resolved IXPE X-ray polarimetric observation of the northwestern rim of SNR RX J1713.7–3946. For the first time, our analysis shows that the magnetic field in the particle acceleration sites of this SNR is oriented tangentially with respect to the shock front. Because of the lack of precise Faraday rotation measurements in the radio band, this was not possible before. The average measured polarization degree (PD) of the synchrotron emission is 12.5% ± 3.3%, lower than the one measured by IXPE in SN 1006, comparable to the Tycho one, but notably higher than the one in Cassiopeia A. On subparsec scales, localized patches within RX J1713.7–3946 display a PD of up to 41.5% ± 9.5%. These results are compatible with a shock-compressed magnetic field. However, in order to explain the observed PD, either the presence of a radial net magnetic field upstream of the shock or partial reisotropization of the turbulence downstream by radial magnetohydrodynamical instabilities can be invoked. From comparison of PD and magnetic field distribution with γ-rays and 12CO data, our results provide new inputs in favor of a leptonic origin of the γ-ray emission.

KW - X-ray astronomy

KW - Polarimetry

KW - Supernova remnants

KW - 1810

KW - 1278

KW - 1667

KW - Astrophysics - High Energy Astrophysical Phenomena

KW - Astrophysics - Astrophysics of Galaxies

UR - https://www.mendeley.com/catalogue/8c197391-32a8-305c-9ac5-1f50ef79f93b/

U2 - 10.3847/2041-8213/ad4a68

DO - 10.3847/2041-8213/ad4a68

M3 - статья

VL - 967

SP - L38

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

ER -

ID: 121642048