Abstract
This contribution summarizes briefly some previous findings based on ISOGAL, MACHO and DENIS observations and goes on to include outlines of two projects now in progress:
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(i)
A complete sample of M stars in the Baade’s Window NGC6522 field is being investigated using the MACHO, ISOGAL, DENIS and 2MASS databases to determine how variability and mass-loss are related to spectral sub-type
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(ii)
The (MACHO) light curves of the defining stars of the infrared LMC mira period-luminosity relations are being analysed to check on their periods and to determine whether new information can reduce the scatter
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© 2003 Springer Science+Business Media Dordrecht
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Glass, I.S. (2003). Characteristics of AGB Stars in the Isogal, Macho and Other Databases. 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_7
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DOI: https://doi.org/10.1007/978-94-010-0139-7_7
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