Abstract
From the near-infrared monitoring observations of intermediate-age clusters, we found that most AGB stars near the tip luminosity are variables in the infrared. It is also suggested that their amplitude may increase with their luminosities
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© 2003 Springer Science+Business Media Dordrecht
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Tanabé, T. et al. (2003). Nir Monitoring of Star Clusters in the Magellanic Clouds. In: Nakada, Y., Honma, M., Seki, M. (eds) Mass-Losing Pulsating Stars and their Circumstellar Matter. Astrophysics and Space Science Library, vol 283. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0139-7_38
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DOI: https://doi.org/10.1007/978-94-010-0139-7_38
Publisher Name: Springer, Dordrecht
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