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Fourteen candidate RR Lyrae star streams in the inner Galaxy

Mateu, C; Read, JI; Kawata, D; (2018) Fourteen candidate RR Lyrae star streams in the inner Galaxy. Monthly Notices of the Royal Astronomical Society , 474 (3) pp. 4112-4129. 10.1093/mnras/stx2937. Green open access

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Abstract

We apply the GC3 stream-finding method to RR Lyrae stars (RRLSs) in the Catalina survey. We find 2 RRLS stream candidates at >4σ confidence and another 12 at >3.5σ confidence over the Galactocentric distance range 4 < D/kpc < 26. Of these, only two are associated with known globular clusters (NGC 1261 and Arp2). The remainder are candidate ‘orphan’ streams, consistent with the idea that globular cluster streams are most visible close to dissolution. Our detections are likely a lower bound on the total number of dissolving globulars in the inner galaxy, since many globulars have few RRLSs, while only the brightest streams are visible over the Galactic RRLS background, particularly given the current lack of kinematical information. We make all of our candidate streams publicly available and provide a new galstreamsPYTHON library for the footprints of all known streams and overdensities in the Milky Way.

Type: Article
Title: Fourteen candidate RR Lyrae star streams in the inner Galaxy
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/stx2937
Publisher version: https://doi.org/10.1093/mnras/stx2937
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: methods: data analysis, astronomical data bases: miscellaneous, stars: variables: RR Lyrae, Galaxy: halo, Galaxy: structure
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10038573
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