Changes between Version 49 and Version 50 of u/zchen/summary


Ignore:
Timestamp:
09/21/16 08:31:49 (8 years ago)
Author:
Zhuo Chen
Comment:

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  • u/zchen/summary

    v49 v50  
    33Model 1 is run on 120 cores and model 2 is run on 240 cores. The normal state of the pulsating AGB star is the same. The mass of the AGB star is always $1M_{\odot}$
    44
    5 || model number || q   || z     || burst || separation ||    link                                                                                                                   || $\dot{m_1}(M_{\odot}/yr)$ || $\dot{m_2}(M_{\odot}/yr)$ || $j_{g}/j_{0}$  ||         accretion/circumbinary disk ||  total gas mass around the binary($M_{\odot}/yr$)  ||
     5|| model number || q   || z     || burst || separation ||    link                                                                                                                   || $\dot{m_1}(M_{\odot}/yr)$ || $\dot{m_2}(M_{\odot}/yr)$ || $j_{g}/j_{0}$  ||         accretion/circumbinary disk ||  total gas mass around the binary($M_{\odot}$)  ||
    66|| 1            || 0.5 || 0.031 ||  no   ||   4AU      ||[https://astrobear.pas.rochester.edu/trac/wiki/u/zchen/summary/model1 model1]  ||      $3.414\times10^{-7}$      ||      $1.157\times10^{-7}$            ||     2.577             ||      Y/Y ||
    77|| 2            || 0.5 || 0.031 ||  yes  ||   4AU      ||[https://astrobear.pas.rochester.edu/trac/wiki/u/zchen/summary/model2 model2]  ||   $3.526\times10^{-7}$     ||    $1.546\times10^{-7}$              ||    2.25             ||  Y/Y ||