Volume 405, Number 2, July II 2003
|Page(s)||577 - 583|
|Section||Galactic structure, stellar clusters, and populations|
|Published online||19 June 2003|
Tracing the Sgr Stream with 2MASS*
Detection of Stream stars around Outer Halo globular clusters
INAF – Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy
2 Observatoire de Strasbourg, 67000 Strasbourg, France e-mail: firstname.lastname@example.org
3 Dipartimento di Astronomia, Università di Bologna, via Ranzani 1, 40127 Bologna, Italy e-mail: email@example.com
4 INAF – Osservatorio Astronomico di Roma, via Frascati 33, 00040 Monte Porzio Catone, Italy e-mail: firstname.lastname@example.org
Corresponding author: M. Bellazzini, email@example.com
Accepted: 24 April 2003
We use infrared Color Magnitude Diagrams from the 2-Micron All-Sky Survey (2MASS) to search for stars belonging to the tidal stream of the Sagittarius dwarf spheroidal galaxy (Sgr dSph) around selected Galactic globular clusters. Statistically significant detections are presented for the cases of Pal 12 and NGC 4147, strongly supporting the idea that these clusters are associated with the Sgr Stream and that they were previous members of the Sgr dSph galaxy.
Key words: Galaxy: halo / Galaxy: structure / globular clusters: individual: Pal 12, NGC 4147
This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.
© ESO, 2003
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.