A Cold Stellar Stream in Pegasus
2019
We report the serendipitous discovery of a
stellarstream in the constellation Pegasus in the south Galactic hemisphere. The
stellarstream was detected using the SDSS Data Release 14 by means of a
matched filterin the color--magnitude diagram that is optimised for a
stellar populationthat is 8 Gyr old with [Fe/H] = $-$0.46 dex, and located at
heliocentricdistance of 18 kpc. The candidate stream is faint (
turnoff pointat $r_0 \sim$ 19.6), sparse and barely visible in SDSS photometry. It is also detected in the (shallower) Pan-STARRs data. The residual
stellar densityin the $(u-g)_0$, $(g-r)_0$
color--
color diagramgives the same estimate for the age and [Fe/H] of this
stellar population. The stream is located at a Galactic coordinates $(l,b) = (79.4,-24.6)$ and extends over 9$^\circ$ (2.5 kpc), with a width of 112 pc. The narrow width suggests a
globular clusterprogenitor.
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