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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 660656.0, MPI für Astronomie / Publikationen_mpia
Spectroscopic hint of a cold stream in the direction of the globular cluster NGC 1851
Authors:Sollima, A.; Gratton, R. G.; Carballo-Bello, J. A.; Martínez-Delgado, D.; Carretta, E.; Bragaglia, A.; Lucatello, S.; Peñarrubia, J.
Date of Publication (YYYY-MM-DD):2012
Journal Abbrev.:Monthly Notices of the Royal Astronomical Society
Volume:426
Issue / Number:2
Start Page:1137
End Page:1143
Audience:Not Specified
Abstract / Description:We present the results of a spectroscopic survey performed in the outskirts of the globular cluster NGC 1851 with VIsible MultiObject Spectrograph (VIMOS)/Very Large Telescope (VLT). The radial velocities of 107 stars in a region between 12 and 33 arcmin around the cluster have been derived. We clearly identify the cluster stellar population over the entire field of view, indicating the presence of a significant fraction of stars outside the tidal radius predicted by King models. We also find tentative evidence of a cold (σv ≤ 20 km s‑1) peak in the distribution of velocities at vr ˜ 180 km s‑1 constituted mainly by main-sequence stars whose location in the colour-magnitude diagram is compatible with a stream at a similar distance to this cluster. If confirmed, this evidence would strongly support the extragalactic origin of this feature. Based on VIsible MultiObject Spectrograph (VIMOS) observations collected with the Very Large Telescope at the European Southern Observatory, Cerro Paranal, Chile, within the observing programme 082.D-0244.Alexander von Humboldt Fellow for Advanced Research.
Free Keywords:methods: data analysis; methods: observational; techniques: radial velocities; globular clusters: individual: NGC 1851; Galaxy: halo; Galaxy: stellar content
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://cdsads.u-strasbg.fr/abs/2012MNRAS.426.1137S
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