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pro vyhledávání: '"Alexander Mushtukov"'
Autor:
Jeremy Heyl, Victor Doroshenko, Denis González-Caniulef, Ilaria Caiazzo, Juri Poutanen, Alexander Mushtukov, Sergey Tsygankov, Demet Kirmizibayrak, Matteo Bachetti, George Pavlov, Iván Agudo, Lucio Antonelli, Luca Baldini, Wayne Baumgartner, Ronaldo Bellazzini, Stefano Bianchi, Stephen Bongiorno, Raffaella Bonino, Alessandro Brez, Niccolò Bucciantini, Fiamma Capitanio, Simone Castellano, Elisabetta Cavazzuti, Chien-Ting Chen, Stefano Ciprini, Enrico Costa, Alessandra De Rosa, Ettore Del Monte, Laura Di Gesu, Niccolo Di Lalla, Alessandro Di Marco, Immacolata Donnarumma, Michal Dovciak, Steven Ehlert, Teruaki Enoto, Yuri Evangelista, Sergio Fabiani, Riccardo Ferrazzoli, Javier Garcia, Shuichi Gunji, Wataru Iwakiri, Svetlana Jorstad, Philip Kaaret, Vladimir Karas, Fabian Kislat, Takao Kitaguchi, Jeffery Kolodziejczak, Henric Krawczynski, Fabio La Monaca, Luca Latronico, Ioannis Liodakis, Simone Maldera, Alberto Manfreda, Frederic Marin, Andrea Marinucci, Alan Marscher, Herman Marshall, Francesco Massaro, Giorgio Matt, Ikuyuki Mitsuishi, Tsunefumi Mizuno, Fabio Muleri, Michela Negro, C.-Y. Ng, Stephen O'Dell, Nicola Omodei, Chiara Oppedisano, Alessandro Papitto, Abel Peirson, Matteo Perri, Melissa Pesce-Rollins, Pierre-Olivier Petrucci, Maura Pilia, Andrea Possenti, Simonetta Puccetti, Brian Ramsey, John Rankin, Ajay Ratheesh, Oliver Roberts, Roger Romani, Carmelo Sgro, Patrick Slane, Paolo Soffitta, Gloria Spandre, Doug Swartz, Toru Tamagawa, Fabrizio Tavecchio, Roberto Taverna, Yuzuru Tawara, Allyn Tennant, Nicholas Thomas, Francesco Tombesi, Alessio Trois, Roberto Turolla, Jacco Vink, Martin Weisskopf, Kinwah Wu, Fei Xie, Silvia Zane
In an X-ray pulsar, a neutron star accretes matter from a stellar companion through an accretion disk. The high magnetic field of the rotating neutron star disrupts the inner edge of the disc, funneling the gas to flow onto the magnetic poles on its
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::162c81a9d5992a1e82599d5236c3b982
https://doi.org/10.21203/rs.3.rs-2887498/v1
https://doi.org/10.21203/rs.3.rs-2887498/v1
One of the models explaining the high luminosity of pulsing ultra-luminous X-ray sources (pULXs) was suggested by Mushtukov et al. (2015). They showed that the accretion columns on the surfaces of highly magnetized neutron stars can be very luminous
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::79b80f1f5283b7d1c8c67fc78806d32c