Disentangling physics and chemistry in AGB outflows: revealing degeneracies when adding complexity

Author:

Van de Sande Marie1ORCID,Walsh Catherine1ORCID,Millar Tom J.2ORCID

Affiliation:

1. School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT, UK

2. Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, University Road, Belfast BT7 1NN, UK

Abstract

The first AGB chemical kinetics model that includes porosity, dust–gas chemistry and companion UV photons, allows us to unravel the interplay of the complexities and identify suites of molecules to determine the presence of a companion star.

Funder

H2020 Marie Skłodowska-Curie Actions

Science and Technology Facilities Council

University of Leeds

Publisher

Royal Society of Chemistry (RSC)

Subject

Physical and Theoretical Chemistry

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Modelling predicts a molecule-rich disc around the AGB star L2 Puppis;Monthly Notices of the Royal Astronomical Society;2024-06-21

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