Outflows from Binary AGB stars with ALMA
Conference contribution, 2014

Binary stars have long been expected to hold the key to the formation of asymmetrical planetary nebulae. With ALMA, we can study the circumstellar outflows from potential precursors in never-before-reached sensitivity and detail. Our pioneering Cycle-0 study of the AGB star R Sculptoris established theoretical predictions and raised new, fundamental questions on the role of binarity in shaping the outflows from evolved stars. In Cycle 1, we have been awarded time to study a small sample of binary AGB stars, for which resolved observations of the binary pairs exist, covering a decisive range in binary separation. We are also preparing a follow-up ALMA proposal of binary planetary nebulae by searching for appropriate CO-emitting candidates with APEX. The current status of and results from these studies will be presented.

stars: planetary nebulae

planetary nebulae: general

Author

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[Person a2eedb84-2110-42bc-9241-7d93804191b6 not found]

Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics

[Person 620ac39d-f3ba-4fd1-ac08-7e13258f4287 not found]

Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics

[Person 9bff6288-5e6e-435a-b34a-ded9f6a07bd4 not found]

[Person b62bd0ec-0a77-4cf7-8255-e4ea9b084d5d not found]

Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics

Asymmetrical Planetary Nebulae VI conference, Proceedings of the conference held 4-8 November, 2013

75-

Subject Categories

Astronomy, Astrophysics and Cosmology

Roots

Basic sciences

More information

Created

10/8/2017