Figure 7 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 7.

Physical HRD for NGC 362. As in Figure 4, candidate strong mass-losing stars are circled in red, and candidate moderate mass-losing stars (excluding s01, a likely cluster nonmember) are marked by purple diamonds (see Table 2). Padova isochrones are also plotted in dark blue for NGC 362, light blue (dashed line) for Galactic stars at a representative distance, and magenta (dashed line) for the SMC. Note that the RGB is cooler than expected.

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