τ1 Aquarii has a stellar classification of B9V; right along the borderline between a B- and A-type main sequence star. It is around 100million years old and has twice the Sun's radius. When examined in the infrared band, it displays an excess emission that is a characteristic of stars with an orbiting debris disk. Indeed, the model that best fits the data suggests there are two concentric circumstellar disks.
WA's premier says he "hasn't been advised" a lack of staffing has led to gaps in the tracking of some alleged domestic violence offenders, despite the Department of Justice actively recruiting to fill roles ... .
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