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Binary Star Stellar Population Synthesis Model For Astrophysical Studies

Published online by Cambridge University Press:  06 January 2014

Z. M. Li ,
C. Y. Mao ,
L. Chen  and
Q. Zhang
Z. M. Li
Affiliation:
Institute for Astronomy and History of Science and Technology, Dali University, China email: zhongmu.li@gmail.com
C. Y. Mao
Affiliation:
Institute for Astronomy and History of Science and Technology, Dali University, China email: zhongmu.li@gmail.com
L. Chen
Affiliation:
Institute for Astronomy and History of Science and Technology, Dali University, China email: zhongmu.li@gmail.com
Q. Zhang
Affiliation:
Institute for Astronomy and History of Science and Technology, Dali University, China email: zhongmu.li@gmail.com
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Abstract

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Binary stars possibly exists in most galaxies and star clusters. Their evolution can lead to significant change in stellar population studies. Binary star to fit group (BS2fit: ∞) has built up a binary star stellar population synthesis model and used it in a few works. This page is to introduce the model and its possible applications.

Keywords

binary starsstellar populationsgalaxiesstar clusters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S298: Setting the scene for Gaia and LAMOST , May 2013 , pp. 422
Copyright
Copyright © International Astronomical Union 2014 

References

Li, Z. M. & Han, Z. W. 2008, MNRAS, 387, 105CrossRefGoogle Scholar
Li, Z. M., Mao, C. Y., Chen, L., & Zhang, Q., 2012, ApJL, 761, L22Google Scholar
Li, Z. M., Mao, C. Y., Chen, L., Zhang, Q. & Li, M. C. 2013, arXiv, 1302.0927Google Scholar