A1 Journal article – refereed

Discovery of the 5 keV Cyclotron Line Followed by Three Harmonics in Swift J1626.6-5156




List of Authors: Molkov S, Doroshenko V, Lutovinov A, Tsygankov S, Santangelo A, Mereminskiy I, Semena A

Publisher: IOP PUBLISHING LTD

Place: Bristol

Publication year: 2021

Journal: Astrophysical Journal Letters

Journal name in source: ASTROPHYSICAL JOURNAL LETTERS

Journal acronym: ASTROPHYS J LETT

Volume number: 915

Number of pages: 8

ISSN: 2041-8205

eISSN: 2041-8213

DOI: http://dx.doi.org/10.3847/2041-8213/ac0c15

URL: https://iopscience.iop.org/article/10.3847/2041-8213/ac0c15


Abstract
We report on observations of the Be/X-ray binary system Swift J1626.6-5156 performed with the Nuclear Spectroscopic Telescope ARray (NuSTAR) during a short outburst in 2021 March, following its detection by the MAXI monitor and Spektrum-Roentgen-Gamma (SRG) observatory. Our analysis of the broadband X-ray spectrum of the source confirms the presence of two absorption-like features at energies E similar to 9 and E similar to 17 keV. These had been previously reported in the literature and interpreted as the fundamental cyclotron resonance scattering feature (CRSF) and its first harmonic (based on Rossi X-ray Timing Explorer (RXTE) data). The better sensitivity and energy resolution of NuSTAR, combined with the low-energy coverage of Neutron star Interior Composition Explorer (NICER), allowed us to detect two additional absorption-like features at E similar to 4.9 keV and E similar to 13 keV. Therefore, we conclude that, in total, four cyclotron lines are observed in the spectrum of Swift J1626.6-5156: the fundamental CRSF at E similar to 4.9 keV and three higher spaced harmonics. This discovery makes Swift J1626.6-5156 the second accreting pulsar, after 4U 0115+63, whose spectrum is characterized by more than three lines of a cyclotronic origin, and implies that the source has the weakest confirmed magnetic field among all X-ray pulsars, B similar to 4 x 10(11) G. This discovery makes Swift J1626.6-5156 one of the prime targets for the upcoming X-ray polarimetry missions covering the soft X-ray band, such as Imaging X-ray Polarimetry Explorer (IXPE) and enhanced X-ray Timing and Polarimetry mission (eXTP).


Last updated on 2021-10-09 at 11:33