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A two-component model for the infrared spectrum of AGB stars

✍ Scribed by Xiong Guan-Zhu; Chen Pei-Sheng; Chen Jian-Bao


Publisher
Elsevier Science
Year
1994
Tongue
English
Weight
70 KB
Volume
18
Category
Article
ISSN
0275-1062

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We propose that the large, radius of $10 3 AU, circumbinary rotating disks observed around some post-asymptotic giant branch (post-AGB) binary stars are formed from slow AGB wind material that is pushed back to the center of the nebula by wide jets. We perform 2D-axisymmetrical numerical simulations