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Tidal Remnants Around the Galactic Globular Clusters NGC1851 and NGC1904

  • Carballo-Bello J
  • Martínez-Delgado D
DOI: 10.1007/978-3-642-11250-8_90
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Abstract

Deep photometry around the Galactic globular clusters NGC 1851 and NGC 1904 obtained with the Wide Field Imager in the 2.2 m ESO telescope reveals a distinct main-sequence of a metal-poor stellar population, consistent with the presence of a very low surface brightness stellar system. The unveiled population might belong to an unknown tidal stream in the Milky Way but other possibilities are here discussed.

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Carballo-Bello, J. A., & Martínez-Delgado, D. (2010). Tidal Remnants Around the Galactic Globular Clusters NGC1851 and NGC1904 (pp. 383–383). https://doi.org/10.1007/978-3-642-11250-8_90

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