Near-ultraviolet detections of four dwarf nova candidates in the
  globular cluster 47 Tucanae
  We investigate near-ultraviolet (NUV) variability in the Galactic globular
cluster (GC) 47 Tucanae (47 Tuc). This work was undertaken within the GC
sub-project of the Transient UV Objects project, a programme which aims to find
and study transient and strongly variable UV sources. Globular clusters are
ideal targets for transient searches because of their high stellar densities
and large populations of variable systems. Using all archival observations of
47 Tuc obtained with the UV/optical telescope (UVOT) aboard the Neil Gehrels
Swift observatory with the uvm2 filter, we searched for UV variability using a
specialised pipeline which utilises difference image analysis. We found four
clear transients, hereafter SW1-4, with positions consistent with those of
known cataclysmic variables (CVs) or CV candidates identified previously using
Hubble Space Telescope observations. All four sources exhibit significant
outbursts. Based on the inferred outburst properties and the association with
known CVs, we tentatively identify the UV transients as CV-dwarf novae (DNe).
Two DNe have been previously observed in 47 Tuc: V2, which has a position
consistent with that of SW4; and AKO 9, which was not in outburst during any of
the UVOT observations. We thus increase the known number of DNe in 47 Tuc to 5
and the total number of detected DNe in all Galactic GCs combined from 14 to
17. We discuss our results in the context of the apparent scarcity of DNe in
GCs. We suggest that the likely cause is observational biases, such as limited
sensitivity due to the high background from unresolved stars in the GC and
limited angular resolution of the telescopes used. We additionally detected one
strongly variable source in 47 Tuc, which could be identified as the known RR
Lyrae star HV 810. We found its period to have significantly increased with
respect to that measured from data taken in 1988.
