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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 5.

SED of source s11, a suspected background galaxy. Black pluses, blue circles, and red circles represent optical/near-IR, Spitzer, and AKARI data, respectively. Wavelength error bars correspond to the filter widths. The scatter in the optical and near-IR photometry is likely due to mismatching of sources, as foreground optical sources may lie directly along the sightline to the galaxy. Four other sources from the galaxy locus in Figure  3 are also shown (green diamonds, purple triangles, orange squares, and blue asterisks), plotted with offset fluxes for visual clarity. The SED of s11 resembles that of the other four background galaxies.

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