Figure 4 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 4.

[3.6] vs. [3.6] − [8] color–magnitude diagram. Lines connect points from each IRAC epoch. The sources identified as candidate stars with strong and moderate mass loss in Figure 3 are marked by red circles and purple diamonds, respectively. The crowded region toward the TRGB is inset at the top right. The source at [8] − [24]>3.5 and M _24 μm < −7 mag in Figure 3 (source s11) is located far from mass-losing AGB stars and near unresolved background galaxies in this CMD. Source s12 may be a background SMC carbon star.

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