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    The MAVERIC Survey: Still No Evidence for Accreting Intermediate-mass Black Holes in Globular Clusters

    267629.pdf (4.130Mb)
    Access Status
    Open access
    Authors
    Tremou, E.
    Strader, J.
    Chomiuk, L.
    Shishkovsky, L.
    Maccarone, T.
    Miller-Jones, James
    Tudor, V.
    Heinke, C.
    Sivakoff, G.
    Seth, A.
    Noyola, E.
    Date
    2018
    Type
    Journal Article
    
    Metadata
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    Citation
    Tremou, E. and Strader, J. and Chomiuk, L. and Shishkovsky, L. and Maccarone, T. and Miller-Jones, J. and Tudor, V. et al. 2018. The MAVERIC Survey: Still No Evidence for Accreting Intermediate-mass Black Holes in Globular Clusters. Astrophysical Journal. 862 (1): Article ID 16.
    Source Title
    Astrophysical Journal
    DOI
    10.3847/1538-4357/aac9b9
    ISSN
    0004-637X
    School
    Curtin Institute of Radio Astronomy (Physics)
    Funding and Sponsorship
    http://purl.org/au-research/grants/arc/FT140101082
    URI
    http://hdl.handle.net/20.500.11937/70037
    Collection
    • Curtin Research Publications
    Abstract

    We present the results of an ultradeep, comprehensive radio continuum survey for the accretion signatures of intermediate-mass black holes (IMBHs) in globular clusters (GCs). The sample, imaged with the Karl G. Jansky Very Large Array and the Australia Telescope Compact Array, comprises 50 Galactic GCs. No compelling evidence for an IMBH is found in any cluster in our sample. In order to achieve the highest sensitivity to low-level emission, we also present the results of an overall stack of our sample as well as various subsamples, also finding nondetections. These results strengthen the idea that IMBHs with masses 1000Me are rare or absent in GCs.

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