Compact protoplanetary disks around the stars of a young binary system
✍ Scribed by Rodríguez, L. F.; D'Alessio, P.; Wilner, D. J.; Ho, P. T. P.; Torrelles, J. M.; Curiel, S.; Gómez, Y.; Lizano, S.; Pedlar, A.; Cantó, J.; Raga, A. C.
- Book ID
- 109702974
- Publisher
- Nature Publishing Group
- Year
- 1998
- Tongue
- English
- Weight
- 263 KB
- Volume
- 395
- Category
- Article
- ISSN
- 0028-0836
- DOI
- 10.1038/26421
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
We have used the James Clerk Maxwell Telescope in Hawaii to search at submillimeter wavelengths for continuum emission from dust, and spectral line emission from carbon monoxide (CO) gas, in the neighborhood of HR 4796A. This young star has a dusty disk with a central cavity, where planets may have
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