Figure 6 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 6.

SED of source s12. The solid black line shows the best fit marcs model (see Section 3.3). The underluminous 3.6 μm flux appears to be the cause of the [3.6] − [8] excess apparent in Figure 4 and may be due to poor photometry or possibly due to absorption from acetylene. AKARI fluxes are systematically too bright, which may be due to stellar blending.

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