Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S343(14), p. 355-356, 2018

DOI: 10.1017/s1743921318006555

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Understanding jets in post-AGB close binaries

Journal article published in 2018 by Dylan Bollen ORCID, Devika Kamath ORCID, Hans Van Winckel, Orsola De Marco ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

AbstractWe have discovered jets in post-AGB binaries. The orbital motion allows us to carry out tomography of the jet as light from the primary star shines through the jet cone. Jets play a major role in many astrophysical environments, from young stellar objects to galaxies. They are also used to study the energetics of accretion phenomena in systems such as red transients and stellar mergers. We use high-resolution, optical, time-series spectra to constrain theories of jet launching, and the impact of jets on the evolution of these post-AGB binaries.

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