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A phenomenological model for the extended zone above AGB stars

โœ Scribed by Noam Soker


Publisher
Elsevier Science
Year
2008
Tongue
English
Weight
156 KB
Volume
13
Category
Article
ISSN
1384-1076

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A model for the formation of large circu
โœ Muhammad Akashi; Noam Soker ๐Ÿ“‚ Article ๐Ÿ“… 2008 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 897 KB

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