E-viri
Recenzirano
Odprti dostop
-
Churazov, Eugene; Khabibullin, Ildar; Thibault Barnouin; Bucciantini, Niccolò; Costa, Enrico; Alessandro Di Marco; Ferrazzoli, Riccardo; man, William; Kaaret, Philip; Kim, Dawoon E; Kolodziejczak, Jeffery J; Kraft, Ralph; Marin, Frédéric; Giorgio, Matt; 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; Bianchi, Stefano; Bongiorno, Stephen D; Bonino, Raffaella; Brez, Alessandro; Capitanio, Fiamma; Castellano, Simone; Cavazzuti, Elisabetta; Chien-Ting, Chen; Ciprini, Stefano; De Rosa, Alessandra; Ettore Del Monte; Niccolò Di Lalla; 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; Kitaguchi, Takao; Krawczynski, Henric; Fabio La Monaca; Latronico, Luca; Liodakis, Ioannis; Maldera, Simone; Manfreda, Alberto; Marinucci, Andrea; Marscher, Alan P; Marshall, Herman L; Massaro, Francesco; Mitsuishi, Ikuyuki; Mizuno, Tsunefumi; Muleri, Fabio; Chi-Yung, Ng; Stephen L. O’Dell; 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; Roberts, Oliver J; Sgrò, Carmelo; Spandre, Gloria; Swartz, Douglas A; Tamagawa, Toru; Tavecchio, Fabrizio; Taverna, Roberto; Tawara, Yuzuru; Thomas, Nicholas E; Tombesi, Francesco; Trois, Alessio; Tsygankov, Sergey S; Turolla, Roberto; Vink, Jacco; Wu, Kinwah; Zane, Silvia
Astronomy and astrophysics (Berlin), 06/2024, Letnik: 686Journal Article
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.
Avtor
![loading ... loading ...](themes/default/img/ajax-loading.gif)
Vnos na polico
Trajna povezava
- URL:
Faktor vpliva
Dostop do baze podatkov JCR je dovoljen samo uporabnikom iz Slovenije. Vaš trenutni IP-naslov ni na seznamu dovoljenih za dostop, zato je potrebna avtentikacija z ustreznim računom AAI.
Leto | Faktor vpliva | Izdaja | Kategorija | Razvrstitev | ||||
---|---|---|---|---|---|---|---|---|
JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
Baze podatkov, v katerih je revija indeksirana
Ime baze podatkov | Področje | Leto |
---|
Povezave do osebnih bibliografij avtorjev | Povezave do podatkov o raziskovalcih v sistemu SICRIS |
---|
Vir: Osebne bibliografije
in: SICRIS
To gradivo vam je dostopno v celotnem besedilu. Če kljub temu želite naročiti gradivo, kliknite gumb Nadaljuj.