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Astrophysics > Solar and Stellar Astrophysics

arXiv:1412.1845 (astro-ph)
[Submitted on 4 Dec 2014 (v1), last revised 14 May 2015 (this version, v2)]

Title:Photometric properties of carbon stars in the Small Magellanic Cloud

Authors:G.C. Sloan, E. Lagadec, K.E. Kraemer, M.L. Boyer, S. Srinivasan, I. McDonald, A.A. Zijlstra
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Abstract:The Optical Gravitational Lensing Experiment identified over 1,800 carbon-rich Mira and semi-regular variables in the Small Magellanic Cloud. Multi-epoch infrared photometry reveals that the semi-regulars and Miras follow different sequences in color-color space when using colors sensitive to molecular absorption bands. The dustiest Miras have the strongest pulsation amplitudes and longest periods. Efforts to determine bolometric magnitudes reveal possible systematic errors with published bolometric corrections.
Comments: 5 pages, 7 figures, contributed talk at "Why Galaxies Care About AGB Stars III", Vienna, July 2014, this http URL Revised arXiv submission includes editorial corrections by R. Wing
Subjects: Solar and Stellar Astrophysics (astro-ph.SR)
Cite as: arXiv:1412.1845 [astro-ph.SR]
  (or arXiv:1412.1845v2 [astro-ph.SR] for this version)
  https://doi.org/10.48550/arXiv.1412.1845

Submission history

From: G. C. Sloan [view email]
[v1] Thu, 4 Dec 2014 21:36:26 UTC (360 KB)
[v2] Thu, 14 May 2015 19:00:14 UTC (360 KB)
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