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LibraryM.L. Boyer (NASA Goddard), K.B.W. McQuinn (Univ. Minnesota), P. Barmby (Univ. W. Ontario), A.Z. Bonanas (National Obs. Athens), R.D. Gehrz (Univ. Minnesota), K.D. Gordon (STScI), M.A.T. Groenewegen (Royal Obs. Belgium), E. Lagadec (Obs. de la Cote d'Azur), D. Lennon (ESA), M. Marengo (Iowa State), I. McDonald (Univ. Manchester), M. Meixner (STScI), E. Skillman (Univ. Minnesota), G.C. Sloan (Cornell), G. Sonneborn (NASA Goddard), J.Th. van Loon (Keele Univ.), A. Zijlstra (Univ. Manchester)
2015, ApJ Supplement, 216, 10
Full manuscript available locally (PDF) or from the arXiv (1412.0695).
The DUSTiNGS survey (DUST in Nearby Galaxies with Spitzer) is a 3.6 and 4.5 µm imaging survey of 50 nearby dwarf galaxies designed to identify dust-producing asymptotic giant branch (AGB) stars and massive stars. Using two epochs, spaced approximately six months apart, we identify a total of 526 dusty variable AGB stars (sometimes called “extreme” or x-AGB stars; [3.6]-[4.5] > 0.1 mag). Of these, 111 are in galaxies with [Fe/H] < -1.5 and 12 are in galaxies with [Fe/H] < -2.0, making them the most metal-poor dust-producing AGB stars known. We compare these identifications to those in the literature and find that most are newly discovered large-amplitude variables, with the exception of ≈30 stars in NGC 185 and NGC 147, 1 star in IC 1613, and 1 star in Phoenix. The chemical abundances of the x-AGB variables are unknown, but the low metallicities suggest that they are more likely to be carbon-rich than oxygen-rich and comparisons with existing optical and near-IR photometry confirm that 70 of the x-AGB variables are confirmed or likely carbon stars. We see an increase in the pulsation amplitude with increased dust production, supporting previous studies suggesting that dust production and pulsation are linked. We find no strong evidence linking dust production with metallicity, indicating that dust can form in very metal-poor environments.
Last modified 25 August, 2016. © Gregory C. Sloan and others.