A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Multiwavelength observations of PSR J2032+4127 during the 2017 periastron passage
Tekijät: Chernyakova M, Malyshev D, Blay P, van Soelen B, Tsygankov S
Kustantaja: OXFORD UNIV PRESS
Julkaisuvuosi: 2020
Journal: Monthly Notices of the Royal Astronomical Society
Tietokannassa oleva lehden nimi: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Lehden akronyymi: MON NOT R ASTRON SOC
Vuosikerta: 495
Numero: 1
Aloitussivu: 365
Lopetussivu: 374
Sivujen määrä: 10
ISSN: 0035-8711
eISSN: 1365-2966
DOI: https://doi.org/10.1093/mnras/staa1181
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/47977389
PSR J2032+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 this paper we present results of optical monitoring of the 2017 periastron passage with the Nordic Optical Telescope. These observations are complemented by X-ray (Swift/XRT, NuSTAR) and GeV (Fermi/LAT) monitoring. Joint analysis of the evolution of the parameters of the H alpha line and the broad-band (X-ray to TeV) spectral shape allows us to propose a model linking the observed emission to the interaction of the pulsar and Be-star winds under the assumption of the inclined disc geometry. Our model allows the observed flux and spectral evolution of the system to be explained in a self-consistent way.
Ladattava julkaisu This is an electronic reprint of the original article. |  |
