Figure 8 from Dust Production and Mass Loss in the Galactic Globular Cluster NGC 362

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Dust Production and Mass Loss in the Galactic Globular Cluster NGC 362

Authors: Martha L. Boyer, Iain McDonald, Jacco Th. van Loon, Karl D. Gordon, Brian Babler, Miwa Block, Steve Bracker, Charles Engelbracht, Joe Hora, Remy Indebetouw, Marilyn Meade, Margaret Meixner, Karl Misselt, Joana M. Oliveira, Marta Sewilo, Bernie Shiao, and Barbara Whitney

BOYER et al. 2009 The Astrophysical Journal 705 746.

Provider: AAS Journals

Caption: Figure 8.

Distribution of candidate mass-losing stars. Most dusty stars are located within the inner 1′ of the cluster center. Red circles mark sources with strong mass loss, and yellow diamonds mark sources experiencing moderate mass loss. The open blue triangle (source s01) is a likely cluster nonmember. Source s11, a background galaxy, falls well outside the field of view shown here.

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