scholarly journals Binary Star Stellar Population Synthesis Model For Astrophysical Studies

2013 ◽  
Vol 9 (S298) ◽  
pp. 422-422
Author(s):  
Z. M. Li ◽  
C. Y. Mao ◽  
L. Chen ◽  
Q. Zhang

AbstractBinary 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.

2020 ◽  
Vol 160 (3) ◽  
pp. 143
Author(s):  
Matthew W. Hosek Jr. ◽  
Jessica R. Lu ◽  
Casey Y. Lam ◽  
Abhimat K. Gautam ◽  
Kelly E. Lockhart ◽  
...  

2008 ◽  
Vol 4 (S252) ◽  
pp. 359-364 ◽  
Author(s):  
Zhongmu Li ◽  
Zhanwen Han

AbstractMore than about 50% stars are in binaries, but the effects of binary evolution were not taken into account in most previous stellar population synthesis studies. In fact, binaries can affect the integrated peculiarities such as spectral energy distributions (SEDs), colours, and line-strength indices of populations. With the effects of binary stars taken into account, some new results for stellar population studies will be shown. We discuss how binaries affect the colours and Lick indices of simple stellar populations, and the measurement of stellar ages and metallicities.


2001 ◽  
Vol 1 ◽  
pp. 145-152
Author(s):  
M. Joly ◽  
C. Boisson ◽  
J. Moultaka ◽  
D. Pelat

2015 ◽  
Vol 449 (3) ◽  
pp. 2853-2874 ◽  
Author(s):  
B. Röck ◽  
A. Vazdekis ◽  
R. F. Peletier ◽  
J. H. Knapen ◽  
J. Falcón-Barroso

New Astronomy ◽  
2019 ◽  
Vol 66 ◽  
pp. 20-30 ◽  
Author(s):  
S. Pasetto ◽  
D. Crnojević ◽  
G. Busso ◽  
C. Chiosi ◽  
L.P. Cassarà

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