Detection of a Nearby Halo Debris Stream in the WISE and 2MASS Surveys
arXiv:1304.1170 · doi:10.1088/2041-8205/769/2/L23
Abstract
Combining the Wide-Field Infrared Survey Explorer All-Sky Release with the 2MASS Point Source Catalog, we detect a nearby, moderately metal-poor stellar debris stream spanning 24 degrees across the southern sky. The stream, which we designate Alpheus, is at an estimated distance of ~1.9 kpc. Its position, orientation, width, estimated metallicity, and to some extent its distance, are in approximate agreement with what one might expect of the leading tidal tail of the southern globular cluster NGC 288.
8 pages, 4 figures, accepted for publication in the Astrophysical Journal Letters
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- Stellar Streams and Clouds in the Galactic Halo
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- Serendipitous Discovery of a Thin Stellar Stream near the Galactic Bulge in the Pan-STARRS1 3Pi Survey
- Spectroscopic Signatures of Extra-Tidal Stars Around the Globular Clusters NGC 6656 (M22), NGC 3201 and NGC 1851 from RAVE
- The Milky Way's stellar streams and globular clusters do not align in a Vast Polar Structure
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- Hunting The Most Distant Stars in the Milky Way: Methods and Initial Results
- The effect of primordial mass segregation on the size scale of globular clusters
- Galactic orbital motions of star clusters: static versus semicosmological time-dependent Galactic potentials
- Tidal stripping stellar substructures around four metal-poor globular clusters in the Galactic bulge
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- An Orbit Fit to Likely Hermus Stream Stars
- A New Tidal Stream Discovered in Gaia DR3
- The mass and redshift dependence of halo star clustering
- Identification of a dwarf galaxy stream in Gaia, and its possible association with the VPOS structure
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