Figure 3 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 3.

[24] vs. [8] − [24] color–magnitude diagram. Lines connect points from each IRAC epoch. Five sources are identified as candidates of strong dusty mass-loss, and five others are candidates for moderate dusty mass loss. One of the moderately dusty candidates is a likely cluster nonmember (source s01).

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