Gamma-ray observations of MAXI J1820+070 during the 2018 outburst

• Verfasst von: Abe, Hyuga [VerfasserIn]
• Verfasst von: Aharonian, Felix A. [VerfasserIn]
• Verfasst von: Ait Benkhali, Faical [VerfasserIn]
• Verfasst von: Bernlöhr, Konrad [VerfasserIn]
• Verfasst von: Ghafourizadeh, Zahra [VerfasserIn]
• Verfasst von: Jankowsky, Felix [VerfasserIn]
• Verfasst von: Hinton, James Anthony [VerfasserIn]
• Verfasst von: Lypova, Iryna [VerfasserIn]
• Verfasst von: Marx, Ramin [VerfasserIn]
• Verfasst von: Quirrenbach, Andreas [VerfasserIn]
• Verfasst von: Steinmaßl, Simon [VerfasserIn]
• Verfasst von: Wagner, Stefan [VerfasserIn]
• Titel: Gamma-ray observations of MAXI J1820+070 during the 2018 outburst
• Körperschaft: MAGIC Collaboration [VerfasserIn]
• Körperschaft: H.E.S.S. Collaboration [VerfasserIn]
• Institutionen: VERITAS Collaboration
• Verf.angabe: Magic Collaboration, H.E.S.S. Collaboration, VERITAS Collaboration
• E-Jahr: 2022
• Jahr: 2022 September 23
• Umfang: 16 S.
• Illustrationen: Illustrationen, Diagramme
• Fussnoten: The Magic Collaboration: H. Abe, S. Abe [und viele weitere], The H.E.S.S. Collaboration: H. Abdalla, F. Aharonian, F. Ait Benkhali, K. Bernlöhr, S. Ghafourizadeh, J.A. Hinton, F. Jankowsky, I. Lypova, R. Marx, A. Quirrenbach, S. Steinmaßl, S.J. Wagner [und viele weitere], The VERITAS Collaboration: V. Bosch-Ramon [und weitere] ; Gesehen am 30.01.2024
• Titel Quelle: Enthalten in: Royal Astronomical SocietyMonthly notices of the Royal Astronomical Society
• Ort Quelle: Oxford : Oxford Univ. Press, 1827
• Jahr Quelle: 2022
• Band/Heft Quelle: 517(2022), 4 vom: Dez., Seite 4736-4751
• ISSN Quelle: 1365-2966
• DOI: doi:10.1093/mnras/stac2686
• Datenträger: Online-Ressource
• Sprache: eng
• K10plus-PPN: 1879520397

Abstract

MAXI J1820+070 is a low-mass X-ray binary with a black hole (BH) as a compact object. This binary underwent an exceptionally bright X-ray outburst from 2018 March to October, showing evidence of a non-thermal particle population through its radio emission during this whole period. The combined results of 59.5 h of observations of the MAXI J1820+070 outburst with the H.E.S.S., MAGIC and VERITAS experiments at energies above 200 GeV are presented, together with Fermi-LAT data between 0.1 and 500 GeV, and multiwavelength observations from radio to X-rays. Gamma-ray emission is not detected from MAXI J1820+070, but the obtained upper limits and the multiwavelength data allow us to put meaningful constraints on the source properties under reasonable assumptions regarding the non-thermal particle population and the jet synchrotron spectrum. In particular, it is possible to show that, if a high-energy (HE) gamma-ray emitting region is present during the hard state of the source, its predicted flux should be at most a factor of 20 below the obtained Fermi-LAT upper limits, and closer to them for magnetic fields significantly below equipartition. During the state transitions, under the plausible assumption that electrons are accelerated up to ∼500 GeV, the multiwavelength data and the gamma-ray upper limits lead consistently to the conclusion that a potential HE and very-HE gamma-ray emitting region should be located at a distance from the BH ranging between 1011 and 1013 cm. Similar outbursts from low-mass X-ray binaries might be detectable in the near future with upcoming instruments such as CTA.