Simultaneous NICER and NuSTAR observations of the ultracompact x-ray binary 4u 1543-624

Ludlam RM, Jaodand AD, Garcia J, Degenaar N, Tomsick JA, Cackett EM, Fabian AC, Gandhi P, Buisson DJK, Shaw AW, Chakrabarty D (2021)


Publication Type: Journal article

Publication year: 2021

Journal

Book Volume: 911

Article Number: abedb0

Journal Issue: 2

DOI: 10.3847/1538-4357/abedb0

Abstract

We present the first joint NuSTAR and NICER observations of the ultracompact X-ray binary (UCXB) 4U 1543 -624 obtained in 2020 April. The source was at a luminosity of L0.5-50 keV = 4.9(D/7 kpc)2 × 1036 erg s-1 and showed evidence of reflected emission in the form of an O VIII line, Fe K line, and Compton hump within the spectrum. We used a full reflection model, known as XILLVERCO, that is tailored for the atypical abundances found in UCXBs, to account for the reflected emission. We tested the emission radii of the O and Fe line components and conclude that they originate from a common disk radius in the innermost region of the accretion disk (Rin . 1.07 RISCO). Assuming that the compact accretor is a neutron star (NS) and the position of the inner disk is the Alfvén radius, we placed an upper limit on the magnetic field strength to be B . 0.7(D/7 kpc) × 108 G at the poles. Given the lack of pulsations detected and position of Rin, it was likely that a boundary layer region had formed between the NS surface and inner edge of the accretion disk with an extent of 1.2 km. This implies a maximum radius of the neutron star accretor of RNS . 12.1 km when assuming a canonical NS mass of 1.4Me.

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APA:

Ludlam, R.M., Jaodand, A.D., Garcia, J., Degenaar, N., Tomsick, J.A., Cackett, E.M.,... Chakrabarty, D. (2021). Simultaneous NICER and NuSTAR observations of the ultracompact x-ray binary 4u 1543-624. Astrophysical Journal, 911(2). https://dx.doi.org/10.3847/1538-4357/abedb0

MLA:

Ludlam, R. M., et al. "Simultaneous NICER and NuSTAR observations of the ultracompact x-ray binary 4u 1543-624." Astrophysical Journal 911.2 (2021).

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