An orphan in the Field of Streams

We use Sloan Digital Sky Survey Data Release 5 photometry and spectroscopy to study a tidal stream that extends over similar to 50 degrees in the north Galactic cap. From the analysis of the path of the stream and the colors and magnitudes of its stars, the stream is similar to 20(-5)(+7) kpc away at its nearest detection (the celestial equator). We detect a distance gradient: the stream is farther away from us at higher declination. The contents of the stream are made up from a predominantly old and metal-poor population that is similar to the globular clusters M13 and M92. The integrated absolute magnitude of the stream stars is estimated to be M-r similar to -7.5. There is tentative evidence for a velocity signature, with the stream moving at similar to-40 km s(-1) at low declinations and similar to + 100 km s(-1) at high declinations. The stream lies on the same great circle as Complex A, a roughly linear association of H I high-velocity clouds stretching over similar to 30 degrees on the sky, and as Ursa Major II, a recently discovered dwarf spheroidal galaxy. Lying close to the same great circle are a number of anomalous, young, and metal-poor globular clusters, including Palomar 1 and Ruprecht 106.