The globular cluster NGC 7492 and the Sagittarius tidal stream: together but unmixed
We have derived from VIMOS spectroscopy the radial velocities for a sample of 71 stars selected from CFHT/Megacam photometry around the Galactic globular cluster NGC 7492. In the resulting velocity distribution, it is possible to distinguish two relevant non-Galactic kinematic components along the s...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
2018
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 474, Issue: 4, Pages: 4766-4771 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx3001 |
| Online Access: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx3001 Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/474/4/4766/4655056 |
| Author Notes: | J.A. Carballo-Bello, J.M. Corral-Santana, M. Catelan, D. Martínez-Delgado, R.R. Muñoz, A. Sollima, C. Navarrete, S. Duffau, P. Côté and M.D. Mora |
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The globular cluster NGC7492 and the Sagittarius tidal stream: together but unmixed
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