http://arxiv.org/abs/1509.07503
Using a shallow, two-color survey carried out with the Dark Energy Camera, we detect the southern, possibly trailing arm of the Orphan Stream. The stream is reliably detected to a declination of $-38^\circ$, bringing the total known length of the Orphan stream to $108^\circ$. We find a slight offset or “S” shape in the stream at $\delta \simeq -14^\circ$ that would be consistent with the transition from leading to trailing arms. This coincides with a moderate concentration of $137 \pm 25$ stars (to $g = 21.6$) that we consider a possible remnant of the Orphan progenitor. The position of this feature is in agreement with previous predictions.
C. Grillmair, L. Hetherington, R. Carlberg, et. al.
Mon, 28 Sep 15
31/67
Comments: 4 pages, 4 figures, accepted for publication in the Astrophysical Journal Letters
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