A Possible Phase-dependent Absorption Feature in the Transient X-Ray Pulsar SAX J2103.5+4545

Brumback MC, Hickox RC, Furst FS, Pottschmidt K, Hemphill P, Tomsick JA, Wilms J, Ballhausen R (2018)


Publication Status: Published

Publication Type: Journal article

Publication year: 2018

Journal

Publisher: IOP PUBLISHING LTD

Book Volume: 852

Article Number: ARTN 132

Journal Issue: 2

DOI: 10.3847/1538-4357/aa9e91

Abstract

We present an X-ray spectral and timing analysis of two Nuclear Spectroscopic Telescope Array (NuSTAR) observations of the transient Be X-ray binary SAX J2103.5+4545 during its 2016 April outburst, which was characterized by the highest flux since NuSTAR's launch. These observations provide detailed hard X-ray spectra of this source during its bright precursor flare and subsequent fainter regular outburst for the first time. In this work, we model the phase-averaged spectra for these observations with a negative and positive power law with an exponential cutoff (NPEX) model and compare the pulse profiles at different flux states. We found that the broadband pulse profile changes from a three-peaked pulse in the first observation to a two-peaked pulse in the second observation, and that each of the pulse peaks has some energy dependence. We also perform pulse-phase spectroscopy and fit phase-resolved spectra with NPEX to evaluate how spectral parameters change with pulse phase. We find that while the continuum parameters are mostly constant with pulse phase, a weak absorption feature at similar to 12 keV might, with further study, be classified as a cyclotron line, does show strong pulse-phase dependence.

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APA:

Brumback, M.C., Hickox, R.C., Furst, F.S., Pottschmidt, K., Hemphill, P., Tomsick, J.A.,... Ballhausen, R. (2018). A Possible Phase-dependent Absorption Feature in the Transient X-Ray Pulsar SAX J2103.5+4545. Astrophysical Journal, 852(2). https://dx.doi.org/10.3847/1538-4357/aa9e91

MLA:

Brumback, M. C., et al. "A Possible Phase-dependent Absorption Feature in the Transient X-Ray Pulsar SAX J2103.5+4545." Astrophysical Journal 852.2 (2018).

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