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An Orphan in the “Field of Streams”
Open accessAbstract
We use Sloan Digital Sky Survey Data Release 5 photometry and spectroscopy to study a tidal stream that extends over ~50° 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 ~20 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 ~ -7.5. There is tentative evidence for a velocity signature, with the stream moving at ~-40 km s -1 at low declinations and ~+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 ~30° 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.
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Citations
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Self-citation
Metadata
- Authors
- Belokurov, V., Evans, N. W., Irwin, M. J., Lynden‐Bell, D., Yanny, B., Vidrih, S., Gilmore, G., Seabroke, G., Zucker, D. B., Wilkinson, M. I., Hewett, P. C., Bramich, D. M., Fellhauer, M., Newberg, H. J., Wyse, R. F. G., Beers, T. C., Bell, E. F., Barentine, J. C., Brinkmann, J., Cole, N., Pan, K., & York, D. G.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2007-03-20
- Volume
- 658
- Issue
- 1
- Pages
- 337-344
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2017509018
- Cited by
- 290
- References
- 41
- FWCI
- 16.71
- Type
- journal article
- Language
- en
- Open access
- bronze
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