| 3 | | 2. Due to the mistake, the mass loss rate was not correct. I think the mass loss rate is crucial in the formation of circumbinary disk. $10^{-7}M_{\odot}/yr$ is somewhat small. If there could be a $10^{-5}M_{\odot}/yr$ AGB wind, the formation of the circumbinary disk will be much more easier. [http://adsabs.harvard.edu/abs/2016A%26A...589A.130L |
| 4 | | Liljegren et al. (2016)] did a detailed study on AGB wind recently. I will try their model. |
| | 3 | 2. Due to the mistake, the mass loss rate was not correct. I think the mass loss rate is crucial in the formation of circumbinary disk. $10^{-7}M_{\odot}/yr$ is somewhat small. If there could be a $10^{-5}M_{\odot}/yr$ AGB wind, the formation of the circumbinary disk will be much more easier. [http://adsabs.harvard.edu/abs/2016A%26A...589A.130L Liljegren et al. (2016)] did a detailed study on AGB wind recently. I will try their model. |
