4.7 Article

The M33 variable star population revealed by spitzer

Journal

ASTROPHYSICAL JOURNAL
Volume 664, Issue 2, Pages 850-861

Publisher

UNIV CHICAGO PRESS
DOI: 10.1086/519068

Keywords

galaxies : individual (M33); galaxies : stellar content; infrared : stars; stars : AGB and post-AGB; stars : variables : other

Funding

  1. Science and Technology Facilities Council [PP/D000955/1] Funding Source: researchfish

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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 mu m. 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 mu m 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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