The M33 Variable Star Population Revealed by Spitzer

  • McQuinn K
  • Woodward C
  • Willner S
  • et al.
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Abstract

We analyze five epochs of Spitzer Space Telescope Infrared Array Camera (IRAC) observations of the nearby spiral galaxy M33. Each epoch covered nearly a square degree at 3.6, 4.5, and 8.0 μm. The point-source catalog from the full data set contains 37,650 stars. The stars have luminosities characteristic of the asymptotic giant branch and can be separated into oxygen-rich and carbon-rich populations by their [3.6]-[4.5] colors. The [3.6]-[8.0] colors indicate that over 80% of the stars detected at 8.0 μm have dust shells. Photometric comparison of epochs using conservative criteria yields a catalog of 2923 variable stars. These variables are most likely long-period variables amid an evolved stellar population. At least one-third of the identified carbon stars are variable.

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McQuinn, K. B. W., Woodward, C. E., Willner, S. P., Polomski, E. F., Gehrz, R. D., Humphreys, R. M., … Fazio, G. G. (2007). The M33 Variable Star Population Revealed by Spitzer. The Astrophysical Journal, 664(2), 850–861. https://doi.org/10.1086/519068

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