Andromeda's dust

B. T. Draine, G. Aniano, Oliver Krause, Brent Groves, Karin Sandstrom, Robert Braun, Adam Leroy, Ulrich Klaas, Hendrik Linz, Hans Walter Rix, Eva Schinnerer, Anika Schmiedeke, Fabian Walter

Research output: Contribution to journalArticle

96 Scopus citations

Abstract

Spitzer Space Telescope and Herschel Space Observatory imaging of M31 is used,with a physical dust model,to construct maps of dust surface density,dust-to-gas ratio,starlight heating intensity,and polycyclic aromatic hydrocarbon (PAH) abundanceout to R 25 kpc.The global dust mass is M d=5.×107M,the global dust/H mass ratio is Md/MH=0.0081,and the global PAH abundance is 〈q PAH〉=0.039.The dust surface density has an inner ring at R=5.6 kpc,a maximum at R=11.2 kpc,and an outer ring at R 15.1 kpc.The dust/gas ratio varies from M d/MH 0.026 at the center to 0.0027 at R 25 kpc. From the dust/gas ratio, we estimate the interstellar medium metallicity to vary by a factor 10, from ZZ3 at R = 0 to 0.3 at R = 25 kpc. The dust heating rate parameter U peaks at the center, with U 35,declining to U 0.25 at R=20 kpc.Within the central kiloparsec,the starlight heating intensity inferred from the dust modeling is close to what is estimated from the stars in the bulge.The PAH abundance reaches a peak qPAH0.045 at R 11.2 kpc.When allowance is made for the different spectrum of the bulge stars,qPAHfor the dust in the central kiloparsec is similar to the overall value of q PAH in the disk.The silicate-graphite-PAH dust model used here is generally able to reproduce the observed dust spectral energy distribution across M31, but overpredicts 500 μm emission at R 2-6 kpc,suggesting that at R=2-6 kpc,the dust opacity varies more steeply with frequency (with β 2.3 between 200 and 600 μm)than in the model.

Original languageEnglish (US)
Article number172
JournalAstrophysical Journal
Volume780
Issue number2
DOIs
StatePublished - Jan 10 2014

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • dust extinction
  • infrared: galaxies
  • infrared:ISM

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    Draine, B. T., Aniano, G., Krause, O., Groves, B., Sandstrom, K., Braun, R., Leroy, A., Klaas, U., Linz, H., Rix, H. W., Schinnerer, E., Schmiedeke, A., & Walter, F. (2014). Andromeda's dust. Astrophysical Journal, 780(2), [172]. https://doi.org/10.1088/0004-637X/780/2/172