A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Discovery of a retrogradely rotating neutron star in the X-ray pulsar GX 301-2
Tekijät: Juhani Mönkkönen, Victor Doroshenko, Sergey S Tsygankov, Armin Nabizadeh, Pavel Abolmasov, Juri Poutanen
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: 494
Numero: 2
Aloitussivu: 2178
Lopetussivu: 2182
Sivujen määrä: 5
ISSN: 0035-8711
eISSN: 1365-2966
DOI: https://doi.org/10.1093/mnras/staa906
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/48444665
We report on the analysis of the spin evolution of a slow X-ray pulsar GX 301-2 along the orbit using long-term monitoring by Fermi/Gamma-ray Burst Monitor. Based on the observationally confirmed accretion scenario and an analytical model for the accretion of angular momentum, we demonstrate that in this system, the neutron star spins retrogradely, that is, in a direction opposite to the orbital motion. This first-of-a-kind discovery of such a system proves the principal possibility of retrograde rotation in accreting systems with suitable accretion torque, and might have profound consequences for our understanding of the spin evolution of X-ray pulsars, estimates of their initial spin periods, and the ultimate result of their evolution.
Ladattava julkaisu This is an electronic reprint of the original article. |  |
