A Spitzer Space Telescope survey of extreme Asymptotic Giant Branch stars in M32

Abstract

We investigate the population of cool, evolved stars in the Local Group dwarf elliptical galaxy M32, using Infrared Array Camera observations from the Spitzer Space Telescope. We construct deep mid-infrared colour-magnitude diagrams for the resolved stellar populations within 3.5 arcmin of M32's centre, and identify those stars that exhibit infrared excess. Our data is dominated by a population of luminous, dust-producing stars on the asymptotic giant branch (AGB) and extend to approximately 3 mag below the AGB tip. We detect for the first time a sizeable population of `extreme' AGB stars, highly enshrouded by circumstellar dust and likely completely obscured at optical wavelengths. The total dust-injection rate from the extreme AGB candidates is measured to be $7.5\times 10^{-7}$ ${\mathrm{M}}_{\odot }{\mathrm{yr}}^{-1}$, corresponding to a gas mass-loss rate of $1.5\times 10^{-4}$ ${\mathrm{M}}_{\odot }{\mathrm{yr}}^{-1}$. These extreme stars may be indicative of an extended star-formation epoch between 0.2 and 5 Gyr ago.

Accepted for publication in MNRAS, 14 pages, 12 figures, 3 tables

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Cited by in corpus (3)

• An Infrared Census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS), II. Discovery of Metal-poor Dusty AGB Stars
• Carbon Stars in the Satellites and Halo of M31
• Infrared variable stars in the compact elliptical galaxy M32