C
Christopher J. Wareing
Researcher at University of Leeds
Publications - 57
Citations - 1239
Christopher J. Wareing is an academic researcher from University of Leeds. The author has contributed to research in topics: Interstellar medium & Planetary nebula. The author has an hindex of 21, co-authored 56 publications receiving 1159 citations. Previous affiliations of Christopher J. Wareing include University of Manchester.
Papers
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The interaction of planetary nebulae and their asymptotic giant branch progenitors with the interstellar medium
TL;DR: In an effort to understand the range of shapes observed in the outer envelopes of PNe, the authors run a comprehensive set of three-dimensional hydrodynamic simulations, from the beginning of the asymptotic giant branch (AGB) superwind phase until the end of the post-AGB/PN phase.
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The interaction of planetary nebulae and their AGB progenitors with the interstellar medium
TL;DR: In an effort to understand the range of shapes observed in the outer envelopes of PNe, the authors run a comprehensive set of three-dimensional hydrodynamic simulations, from the beginning of the asymptotic giant branch (AGB) superwind phase until the end of the post-AGB/PN phase.
Journal ArticleDOI
Experimental measurement and Reynolds-averaged Navier–Stokes modelling of the near-field structure of multi-phase CO2 jet releases
Robert M. Woolley,Michael Fairweather,Christopher J. Wareing,Samuel A.E.G. Falle,Christophe Proust,Jérôme Hebrard,Didier Jamois +6 more
TL;DR: In this article, a computational fluid dynamic model capable of accurately representing the complex physics observed in such a release, essential if dispersion phenomena are to be accurately predicted, is presented. But the model is not suitable for the modeling of CO 2 pipelines and intermediate storage vessels.
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Vortices in the Wakes of Asymptotic Giant Branch Stars
TL;DR: In this article, the authors simulated the wind from an asymptotic giant branch (AGB) star moving through and sweeping up its surrounding interstellar medium (ISM), and found vortices on the size scale of 10-1 to 101 pc in the wake of the star.
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It’s a Wonderful Tail: The Mass-Loss History of Mira
TL;DR: In this paper, the authors successfully hydrodynamically modeled the bow shock and tail as the interaction between the asymptotic giant branch (AGB) wind launched from Mira A and the surrounding interstellar medium.