Abstract
The main objectives of our project on super metal rich stars (SMR) are the following:
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1.
to perform population synthesis of stellar aggregates;
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2.
to provide a complete stellar library as input for 1.;
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3.
to calibrate SMR, stars in terms of atmospheric parameters;
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4.
to compute synthetic spectral indices.
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References
Alonso, A., Arribas, S., Martínez-Roger, C. 1996, A&A 313, 873
Chavez, M., 1995, PhD Thesis, SISSA
Chavez, M., Malagnini, M.L., Morossi, C. 1995, Ap.J. 440, 210
Chavez, M., Buzzoni, A., Malagnini, M.L., Morossi, C. 1996a, in “Fresh Views of Elliptical Galaxies”, ASP Conf. Ser. 86 (eds. A.Buzzoni, A. Renzini, A. Serrano) p. 249
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© 2000 Springer Science+Business Media Dordrecht
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Malagnini, M.L., Morossi, C., Buzzoni, A., Chavez, M. (2000). Observations of Candidate SMR Stars. In: Matteucci, F., Giovannelli, F. (eds) The Evolution of The Milky Way. Astrophysics and Space Science Library, vol 255. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0938-6_7
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DOI: https://doi.org/10.1007/978-94-010-0938-6_7
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