Multi-wavelength observations of PSRJ 2032+4127 during the 2017 periastron passage

PSRJ 2032+4127 is only the second known gamma-ray binary where it is confirmed that a young radio pulsar is in orbit around a Be-star. The interaction of the pulsar wind with the mass outflow from the companion leads to broad band emission from radio up to TeV energies. In the current paper we prese...

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Veröffentlicht in:	arXiv.org 2020-04
Hauptverfasser:	Chernyakova, Maria, Malyshev, Denys, Blay, Pere, Brian van Soelen, Tsygankov, Sergey
Format:	Artikel
Sprache:	eng
Schlagworte:	Broadband Companion stars Emission Evolution Gamma rays Monitoring Physics - High Energy Astrophysical Phenomena Pulsars Stellar winds
Online-Zugang:	Volltext
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