Figure 9 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 9.

SEDs of moderately dusty stars at the TRGB in NGC 362. Wavelength error bars correspond to the filter width. AKARI data are plotted as red squares and Spitzer data are plotted as blue circles. marcs models are solid black lines. IRAC epoch 1 is plotted with open blue circles, and IRAC epoch 2 is plotted with closed blue circles. All four stars are well fit by a dusty silicate model (magenta, dotted line), but s09 is fit equally well by a dusty AMC model (green, dashed line).

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