Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 512, Issue 4, Pages 5037-5066Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stac756
Keywords
radio continuum: galaxies; radio continuum: general
Categories
Funding
- European Research Council (ERC) under the European Union [694745]
- UnivEarthS Labex program of Universite Sorbonne Paris Cite [ANR-10-LABX-0023, ANR-11-IDEX-0005-02]
- National Research Foundation (NRF)
- University of Cape Town (UCT)
- I-CORE Program of the Planning and Budgeting Committee
- Israel Science Foundation
- ISF [647/18]
- GIF, the German-Israeli Foundation for Scientific Research and Development
- United States-Israel Binational Science Foundation (BSF) [2018154]
- National Research Foundation of South Africa [93405, 119446]
- GIF
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In this article, we present 21 new long-term variable radio sources discovered during 2 years of weekly monitoring of the low-mass X-ray binary GX 339-4 using MeerKAT. These sources exhibit variability on time-scales ranging from weeks to months, with a variety of light-curve shapes and spectral index properties. The cause of the variability is likely refractive scintillation of active galactic nuclei in most cases.
We present 21 new long-term variable radio sources found commensally in 2 yr of weekly MeerKAT monitoring of the low-mass X-ray binary GX 339-4. The new sources are vary on time-scales of weeks to months and have a variety of light-curve shapes and spectral index properties. Three of the new variable sources are coincident with multiwavelength counterparts; and one of these is coincident with an optical source in deep MeerLICHT images. For most sources, we cannot eliminate refractive scintillation of active galactic nuclei as the cause of the variability. These new variable sources represent 2.2 +/- 0.5 per cent of the unresolved sources in the field, which is consistent with the 1-2 per cent variability found in past radio variability surveys. However, we expect to find short-term variable sources in the field and these 21 new long-term variable sources. We present the radio light curves and spectral index variability of the new variable sources, as well as the absolute astrometry and matches to coincident sources at other wavelengths.
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