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Population of AGB stars in the outer Galaxy
Published online by Cambridge University Press: 30 December 2019
Abstract
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We present preliminary results of a study aimed at identifying and characterizing the Asymptotic Giant Branch (AGB) stars in the outer Galaxy using the color-color diagram (CCD) that combines the Spitzer Space Telescope and 2MASS photometry: Ks – [8.0] vs. Ks – [24]. Our initial study concentrates on a region in the outer Galactic plane around a galactic longitude l of 105°, where we identified 777 O-rich and 200 C-rich AGB star candidates.
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- © International Astronomical Union 2019
References
Matsuura, M., Bernard-Salas, J., Lloyd Evans, T., et al. 2014 MNRAS, 439, 1472
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Szczerba, R., Bosco, H.K.Y., Sewiło, M., Siódmiak, N., & Karska, A. 2016, Journal of Physics: Conference Series, Volume 728, Issue 4, article id. 042004CrossRefGoogle Scholar
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