A Spitzer Space Telescope Atlas of ω Centauri: The Stellar Population, Mass Loss, and the Intracluster Medium

Details A Spitzer Space Telescope Atlas of ω Centauri: The Stellar Population, Mass Loss, and the Intracluster Medium A Spitzer Space Telescope Atlas of ω Centauri: The Stellar Population, Mass Loss, and the Intracluster Medium

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.5807b&link_type=abstract

American Astronomical Society, AAS Meeting #211, #58.07; Bulletin of the American Astronomical Society, Vol. 39, p.834

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a Spitzer Space Telescope imaging survey of the most massive Galactic globular cluster, ω Centauri, and investigate stellar mass loss at low metallicity and the intracluster medium (ICM). The survey covers approximately 3.2× the cluster half-mass radius at 3.6, 4.5, 5.8, 8, and 24 μm, resulting in a catalog of over 22,000 point-sources in the cluster. Approximately 350 cluster members show a red excess at 24 μm, indicative of circumstellar dust. If all of the dusty sources are experiencing mass loss, the cumulative rate of loss is estimated at 1.3 - 1.8 × 10-6 M&sun;/yr, 15% - 30% of which is supplied by three asymptotic giant branch stars at the tip of the red giant branch. If this material had remained in the cluster center, its dust component (> 4 × 10-4 M&sun;) would be detectable in our 24 μm images. While no dust cloud located at the center of ω Cen is apparent, we do see four regions of very faint, diffuse emission beyond two half-mass radii at 24 μm. It is unclear whether these dust clouds are foreground emission or are associated with ω Cen. In the latter case, these clouds may be the ICM in the process of escaping from the cluster.
This work is supported in part by NASA through Spitzer contracts
1276760, 1256406, and 1215746 issued by JPL/Caltech to the University of Minnesota

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