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

Author:

Tudor Vlad1ORCID,Miller-Jones James C A1ORCID,Strader Jay2,Bahramian Arash1ORCID,Shishkovsky Laura2,Plotkin Richard M3ORCID,Chomiuk Laura2,Heinke Craig O4ORCID,Maccarone Thomas J5,Sivakoff Gregory R4,Tremou Evangelia6ORCID,Anderson Gemma E1ORCID,Russell Thomas D7ORCID,Tzioumis Anastasios K8

Affiliation:

1. International Centre for Radio Astronomy Research, Curtin University , GPO Box U1987, Perth, WA 6845, Australia

2. Center for Data Intensive and Time Domain Astronomy, Department of Physics and Astronomy, Michigan State University , East Lansing, MI 48824, USA

3. Department of Physics, University of Nevada , Reno, NV 89557, USA

4. Department of Physics, University of Alberta , CCIS 4-183, Edmonton, AB T6G 2E1, Canada

5. Department of Physics, Texas Tech University , Box 41051, Science Building, Lubbock, TX 79409, USA

6. LESIA, Observatoire de Paris, CNRS, PSL Research University, Sorbonne Universite, Universite de Paris , Meudon F-92190, France

7. INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica , Via U. La Malfa 153, I-90146 Palermo, Italy

8. Australia Telescope National Facility, CSIRO , PO Box 76, Epping, New South Wales 1710, Australia

Abstract

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.

Funder

Curtin University

Australian Research Council

National Science Foundation

National Aeronautics and Space Administration

Packard Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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