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This is a very short period system, which is dominated by emission
from the white dwarf, a clear sign for a low accretion rate. No
evidence for the secondary, so it might contain a brown dwarf
donor. The system is grazingly eclipsing. We expect that it belongs to
the WZ Sge stars, having extremely infrequent outbursts (no outburst
detected so far), but monitoring will be necessary to confirm this
hypothesis. If it has outbursts similar to WZ Sge, it could easily
reach 10th magnitude.
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