MKT J170456.2-482100 the first transient discovered by MeerKAT

Open Access
Authors
  • L.N. Driessen
  • I. McDonald
  • D.A.H. Buckley
  • M. Caleb
Publication date 01-2020
Journal Monthly Notices of the Royal Astronomical Society
Volume | Issue number 491 | 1
Pages (from-to) 560-575
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract
We report the discovery of the first transient with MeerKAT, MKT J170456.2–482100, discovered in ThunderKAT images of the low-mass X-ray binary GX339–4. MKT J170456.2–482100 is variable in the radio, reaching a maximum flux density of 0.71±0.11mJy on 2019 October 12, and is undetected in 15 out of 48 ThunderKAT epochs. MKT J170456.2–482100 is coincident with the chromospherically active K-type sub-giant TYC 8332-2529-1, and ∼18yr of archival optical photometry of the star shows that it varies with a period of 21.25±0.04d⁠. The shape and phase of the optical light curve changes over time, and we detect both X-ray and UV emission at the position of MKT J170456.2–482100, which may indicate that TYC 8332-2529-1 has large star spots. Spectroscopic analysis shows that TYC 8332-2529-1 is in a binary, and has a line-of-sight radial velocity amplitude of 43kms−1⁠. We also observe a spectral feature in antiphase with the K-type sub-giant, with a line-of-sight radial velocity amplitude of ∼12±10kms−1⁠, whose origins cannot currently be explained. Further observations and investigation are required to determine the nature of the MKT J170456.2–482100 system.
Document type Article
Note This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2019 The Author(s) published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Language English
Published at https://doi.org/10.1093/mnras/stz3027
Other links https://ui.adsabs.harvard.edu/abs/2020MNRAS.491..560D/abstract
Downloads
MKT J170456.2−482100 (Final published version)
Permalink to this page
Back