Hostname: page-component-7479d7b7d-t6hkb Total loading time: 0 Render date: 2024-07-11T08:38:48.181Z Has data issue: false hasContentIssue false
  • English
  • Français

The onset of mass loss in AGB stars

Published online by Cambridge University Press:  30 December 2019

Iain McDonald Open the ORCID record for Iain McDonald [Opens in a new window]
Iain McDonald*
Affiliation:
Jodrell Bank Centre for Astrophysics, University of Manchester, Manchester, M13 9PL, UK email: iain.mcdonald-2@manchester.ac.uk
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The factors controlling strong mass loss from evolved stars remain elusive, frustrating efforts to parameterise mass loss in models of evolved stars. We herein describe evidence we have collected to show that the mass-loss rate of stars is controlled by stellar pulsations, and that we are close to providing improved prescriptions for mass-loss rates from many kinds of evolved stars.

Keywords

stars: mass lossstars: AGB and post-AGBstars: variables: othercircumstellar matterstars: evolutionstars: late-typestars: chromospheresstars: magnetic fieldsstars: Population IIstars: windsoutflows
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S343: Why Galaxies Care About AGB Stars: A Continuing Challenge through Cosmic Time , August 2018 , pp. 464 - 465
Copyright
© International Astronomical Union 2019 

References

Dupree, A.K., Hartmann, L., & Avrett, E.H. 1984, ApJ, 281, L37 10.1086/184280CrossRefGoogle Scholar
Groenewegen, M.A.T. 2014, A&A, 561, L11 Google Scholar
Groenewegen, M.A.T., et al. 2016, A&A, 596, A50 Google Scholar
Handberg, R., et al. 2017, MNRAS, 472, 979 10.1093/mnras/stx1929CrossRefGoogle Scholar
Höfner, S., & Olofsson, H. 2018, AARv, 26, 1 Google Scholar
McDonald, I., Zijlstra, A.A., & Boyer, M.L. 2012, MNRAS, 427, 343 10.1111/j.1365-2966.2012.21873.xCrossRefGoogle Scholar
McDonald, I., et al. 2014, MNRAS, 439, 2618 10.1093/mnras/stu117CrossRefGoogle Scholar
McDonald, I., & Zijlstra, A.A. 2015, MNRAS, 448, 502 10.1093/mnras/stv007CrossRefGoogle Scholar
McDonald, I., et al. 2015, MNRAS, 453, 4324 10.1093/mnras/stv1968CrossRefGoogle Scholar
McDonald, I., & Zijlstra, A.A. 2016, ApJ, 823, L38 10.3847/2041-8205/823/2/L38CrossRefGoogle Scholar
McDonald, I., et al. 2016, MNRAS, 456, 4542 10.1093/mnras/stv2942CrossRefGoogle Scholar
McDonald, I., Zijlstra, A.A., & Watson, R.A. 2017, MNRAS, 471, 770 10.1093/mnras/stx1433CrossRefGoogle Scholar
Miglio, A., et al. 2012, MNRAS, 419, 2077 10.1111/j.1365-2966.2011.19859.xCrossRefGoogle Scholar
Reimers, D. 1975, Mem. Soc. Royale Sci. Liège, 8, 369 Google Scholar
Renzini, A., & Voli, M. 1975, A&A, 94, 175 Google Scholar
Trabucchi, M., et al. 2017, ApJ, 847, 139 10.3847/1538-4357/aa8998CrossRefGoogle Scholar