Hostname: page-component-6bf8c574d5-w79xw Total loading time: 0 Render date: 2025-02-17T15:40:02.274Z Has data issue: false hasContentIssue false
  • English
  • Français

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: [email protected]
C. Y. Mao
Affiliation:
Institute for Astronomy and History of Science and Technology, Dali University, China email: [email protected]
L. Chen
Affiliation:
Institute for Astronomy and History of Science and Technology, Dali University, China email: [email protected]
Q. Zhang
Affiliation:
Institute for Astronomy and History of Science and Technology, Dali University, China email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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