The heating of dust by old stellar populations in the bulge of M31

Brent Groves, Oliver Krause, Karin Sandstrom, Anika Schmiedeke, Adam Leroy, Hendrik Linz, Maria Kapala, Hans Walter Rix, Eva Schinnerer, Fatemeh Tabatabaei, Fabian Walter, Elisabete da Cunha

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84 Citations (Scopus)

Abstract

We use new Herschel multiband imaging of the Andromeda galaxy to analyse how dust heating occurs in the central regions of galaxy spheroids that are essentially devoid of young stars. We construct a dust temperature map of M31 through fitting modified blackbodies to the Herschel data, and find that the temperature within 2kpc rises strongly from the mean value in the disc of 17 ± 1 to ∼35K at the centre. Ultraviolet (UV) to near-infrared (IR) imaging of the central few kpc shows directly the absence of young stellar populations, delineates the radial profile of the stellar density and demonstrates that even the near-UV dust extinction is optically thin in M31's bulge. This allows the direct calculation of the stellar radiation heating in the bulge, U *(r), as a function of radius. The increasing temperature profile in the centre matches that expected from the stellar heating, i.e. that the dust heating and cooling rates track each other over nearly two orders of magnitude in U *. The modelled dust heating is in excess of the observed dust temperatures, suggesting that it is more than sufficient to explain the observed IR emission. Together with the wavelength-dependent absorption cross-section of the dust, this demonstrates directly that it is the optical, not UV, radiation that sets the heating rate. This analysis shows that neither young stellar populations nor stellar near-UV radiation is necessary to heat dust to warm temperatures in galaxy spheroids. Rather, it is the high densities of Gyr-old stellar populations that provide a sufficiently strong diffuse radiation field to heat the dust. To the extent which these results pertain to the tenuous dust found in the centres of early-type galaxies remains yet to be explored.

Original languageEnglish
Pages (from-to)892-902
Number of pages11
JournalMonthly Notices of the Royal Astronomical Society
Volume426
Issue number2
DOIs
Publication statusPublished - 21 Oct 2012
Externally publishedYes

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