Zobrazeno 1 - 10
of 776
pro vyhledávání: '"PSR B1259–63"'
Autor:
Chernyakova, M., Malyshev, D., van Soelen, B., Gallagher, A. Finn, Matchett, N., Russell, T. D., Eijnden, J. van den, Lower, M. E., Johnston, S., Tsygankov, S., Salganik, A., Shebalkova, Iu.
PSR B1259-63 is a gamma-ray binary system with a 48 ms radio pulsar orbiting around an O9.5Ve star, LS 2883, in a highly eccentric ~3.4 yr long orbit. Close to the periastron the system is detected from radio up to the TeV energies due to the interac
Externí odkaz:
http://arxiv.org/abs/2411.02128
Autor:
Kaaret, Philip, Roberts, Oliver J., Ehlert, Steven R., Swartz, Douglas A., Weisskopf, Martin C., Liodakis, Ioannis, Saade, M. Lynne, O'Dell, Stephen L., Chen, Chien-Ting
Some X-ray binaries containing an energetic pulsar in orbit around a normal star accelerate particles to high energies in the shock cone formed where the pulsar and stellar winds collide. The magnetic field geometry in the acceleration region in such
Externí odkaz:
http://arxiv.org/abs/2409.16116
PSR B1259-63 is a gamma-ray binary system with a radio pulsar orbiting an O9.5Ve star, LS 2883, with a period of ~3.4 yr. Close to the periastron the system is detected at all wavelengths, from radio to the TeV energies. The emission in this time per
Externí odkaz:
http://arxiv.org/abs/2309.08299
Akademický článek
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Akademický článek
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Publikováno v:
Universe 2021, 7(12), 472
PSR B1259-63 is a $\gamma$-ray binary system, where the compact object is a pulsar. The system has an orbital period of 1236.7 days and shows peculiar $\gamma$-ray flares (in 100\,MeV--300\,GeV) after its periastron time. We analyzed the \textit{Ferm
Externí odkaz:
http://arxiv.org/abs/2112.02295
Autor:
Chernyakova, Maria, Malyshev, Denys, van Soelen, Brian, O'Sullivan, Shane, Sobey, Charlotte, Tsygankov, S., Keague, Samuel Mc., Green, Jacob, Kirwan, Matthew, Santangelo, Andrea, Pühlhofer, Gerd, Monageng, Itumeleng M.
PSR B1259-63 is a gamma-ray binary system hosting a radio pulsar orbiting around a O9.5Ve star, LS 2883, with a period of ~3.4 years. The interaction of the pulsar wind with the LS 2883 outflow leads to unpulsed broadband emission in the radio, X-ray
Externí odkaz:
http://arxiv.org/abs/2106.03759
Autor:
Chernyakova, M., Malyshev, D., Keague, S. Mc, van Soelen, B., Marais, J. P., Martin-Carrillo, A., Murphy, D.
PSR B1259-63 is a gamma-ray binary system hosting a radio pulsar orbiting around a O9.5Ve star, LS 2883, with a period of ~3.4 years. The interaction of the pulsar wind with the LS 2883 outflow leads to unpulsed broad band emission in the radio, X-ra
Externí odkaz:
http://arxiv.org/abs/2005.14060
Autor:
Philip Kaaret, Oliver J. Roberts, Steven R. Ehlert, Douglas A. Swartz, Martin C. Weisskopf, Ioannis Liodakis, M. Lynne Saade, Stephen L. O’Dell, Chien-Ting Chen
Publikováno v:
The Astrophysical Journal Letters, Vol 974, Iss 1, p L1 (2024)
Some X-ray binaries containing an energetic pulsar in orbit around a normal star accelerate particles to high energies in the shock cone formed where the pulsar and stellar winds collide. The magnetic field geometry in the acceleration region in such
Externí odkaz:
https://doaj.org/article/d213a656eb9a4cb0b583a0f1cff418f3
Autor:
Miller-Jones, James C. A., Deller, Adam T., Shannon, Ryan M., Dodson, Richard, Moldón, Javier, Ribó, Marc, Dubus, Guillaume, Johnston, Simon, Paredes, Josep M., Ransom, Scott M., Tomsick, John A.
The pulsar/massive star binary system PSR B1259-63 / LS 2883 is one of the best-studied gamma-ray binaries, a class of systems whose bright gamma-ray flaring can provide important insights into high-energy physics. Using the Australian Long Baseline
Externí odkaz:
http://arxiv.org/abs/1804.08402