Abstract
Results of the Vassiliadis and Wood (1993) model for the evolution on the AGB are used to study how DENIS can complement an optical and IRAS based study of Long Period Variable AGB stars in a field towards the galactic bulge.
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References
Blommaert, J.A.D.L.: 1992, Ph D thesis, Leiden University
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Szczerba, R. and Blommaert, J.A.D.L.: 1993, in “Planetary Nebulae Nuclei Evolution: Models versus Observations”, Acta Astronomica, in press
Vassiliadis, E., Wood, P.R.: 1993, AJ 413, 641
Wesselink, T.J.H.: 1987, Ph.D. Thesis, Catholic University of Nijmegen
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© 1994 Springer Science+Business Media Dordrecht
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Blommaert, J.A.D.L., Szczerba, R. (1994). The Evolution from Visible to Infrared Variable AGB Stars. In: Epchtein, N., Omont, A., Burton, B., Persi, P. (eds) Science with Astronomical Near-Infrared Sky Surveys. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0946-8_30
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DOI: https://doi.org/10.1007/978-94-011-0946-8_30
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