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Jones, O. C.; Nally, C.; Sharp, M. J.; McDonald, Iain; Boyer, M. L.; Meixner, M.; Kemper, F.; Ferguson, A .M. N.; Goldman, S. R. and Rich, R. M.
(2021).
DOI: https://doi.org/10.1093/mnras/stab923
Abstract
Variable stars in the compact elliptical galaxy M32 are identified, using three epochs of photometry from the Spitzer Space Telescope at 3.6 and 4.5 μm, separated by 32 to 381 days. We present a high-fidelity catalogue of sources detected in multiple epochs at both 3.6 and 4.5 μm, which we analysed for stellar variability using a joint probability error-weighted flux difference. Of these, 83 stars are identified as candidate large-amplitude, long-period variables, with 28 considered high-confidence variables. The majority of the variable stars are classified as asymptotic giant branch star candidates using colour-magnitude diagrams. We find no evidence supporting a younger, infrared-bright stellar population in our M32 field.
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About
- Item ORO ID
- 76272
- Item Type
- Journal Item
- ISSN
- 1365-2966
- Project Funding Details
-
Funded Project Name Project ID Funding Body Not Set ST/L000768/1 STFC (Science & Technology Facilities Council) - Keywords
- stars: late-type – galaxies: individual (M32) – galaxies: stellar content – infrared: galaxies – infrared: stars; stars: AGB and post-AGB
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Copyright Holders
- © 2021 The Authors
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