Abstract / Description of output
We report the discovery of a thin stellar stream found in Pan-STARRS1
photometry near the Galactic bulge in the constellation of Ophiuchus. It
appears as a coherent structure in the colour-selected stellar density
maps produced to search for tidal debris around nearby globular
clusters. The stream is exceptionally short and narrow; it is about
2.5° long and 6 arcmin wide in projection. The colour-magnitude
diagram of this object, which harbours a blue horizontal-branch, is
consistent with an old and relatively metal-poor population ([Fe/H]
˜-1.3) located 9.5 ± 0.9 kpc away at (l, b) ˜
(5°, +32°), and 5.0 ± 1.0 kpc from the Galactic centre.
These properties argue for a globular cluster as progenitor. The finding
of such a prominent, nearby stream suggests that many streams could
await discovery in the more densely populated regions of our Galaxy.
Original language | English |
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Journal | Monthly Notices of the Royal Astronomical Society: Letters |
Volume | 443 |
DOIs | |
Publication status | Published - 1 Sept 2014 |
Keywords / Materials (for Non-textual outputs)
- surveys
- globular clusters: general
- Galaxy: halo
- Galaxy: structure
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Annette Ferguson, FRSE
- School of Physics and Astronomy - Personal Chair in Observational Astrophysics
Person: Academic: Research Active