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- W2885087126 abstract "Aims . We explore the wealth of high-quality photometric data provided by data release 2 (DR2) of the Gaia mission for long-period variables (LPVs) in the Large Magellanic Cloud (LMC). Our goal is to identify stars of various types and masses along the asymptotic giant branch. Methods . For this endeavour, we developed a new multi-band approach combining Wesenheit functions W RP,BP−RP and W K s , J − K s in the Gaia BP, RP, and 2MASS J, K s spectral ranges, respectively, and use a new diagram, ( W RP,BP−RP − W K s , J − K s ) versus K s , to distinguish between different kinds of stars in our sample of LPVs. We used stellar population synthesis models to validate our approach. Results . We demonstrate the ability of the new diagram to discriminate between O- and C-rich objects, and to identify low-mass, intermediate-mass, and massive O-rich red giants, as well as extreme C-rich stars. Stellar evolution and population synthesis models guide the interpretation of the results, highlighting the diagnostic power of the new tool to discriminate between stellar initial masses, chemical properties, and evolutionary stages." @default.
- W2885087126 created "2018-08-22" @default.
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- W2885087126 date "2018-08-01" @default.
- W2885087126 modified "2023-09-24" @default.
- W2885087126 title "A new method to identify subclasses among AGB stars using <i>Gaia</i> and 2MASS photometry" @default.
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- W2885087126 doi "https://doi.org/10.1051/0004-6361/201833615" @default.
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