The MAVERIC survey: a catalogue of radio sources in southern globular clusters from the Australia Telescope Compact Array

ABSTRACT Radio continuum observations offer a new window on compact objects in globular clusters compared to typical X-ray or optical studies. As part of the MAVERIC survey, we have used the Australia Telescope Compact Array to carry out a deep (median central noise level ≈4 $\mu$Jy beam-1) radio co...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2022-05, Vol.513 (3), p.3818-3835
Hauptverfasser: Tudor, Vlad, Miller-Jones, James C A, Strader, Jay, Bahramian, Arash, Shishkovsky, Laura, Plotkin, Richard M, Chomiuk, Laura, Heinke, Craig O, Maccarone, Thomas J, Sivakoff, Gregory R, Tremou, Evangelia, Anderson, Gemma E, Russell, Thomas D, Tzioumis, Anastasios K
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Sprache:eng
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Zusammenfassung:ABSTRACT Radio continuum observations offer a new window on compact objects in globular clusters compared to typical X-ray or optical studies. As part of the MAVERIC survey, we have used the Australia Telescope Compact Array to carry out a deep (median central noise level ≈4 $\mu$Jy beam-1) radio continuum survey of 26 southern globular clusters at central frequencies of 5.5 and 9.0 GHz. This paper presents a catalogue of 1285 radio continuum sources in the fields of these 26 clusters. Considering the surface density of background sources, we find significant evidence for a population of radio sources in seven of the 26 clusters, and also identify at least 11 previously known compact objects (six pulsars and five X-ray binaries). While the overall density of radio continuum sources with 7.25-GHz flux densities ≳ 20 $\mu$Jy in typical globular clusters is relatively low, the survey has already led to the discovery of several exciting compact binaries, including a candidate ultracompact black hole X-ray binary in 47 Tuc. Many of the unclassified radio sources near the centres of the clusters are likely to be true cluster sources, and multiwavelength follow-up will be necessary to classify these objects and better understand the demographics of accreting compact binaries in globular clusters.
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stac1034