Hostname: page-component-76fb5796d-qxdb6 Total loading time: 0 Render date: 2024-04-28T09:06:14.058Z Has data issue: false hasContentIssue false
  • English
  • Français

The onset of mass loss in evolved stars

Published online by Cambridge University Press:  30 November 2022

Iain McDonald Open the ORCID record for Iain McDonald [Opens in a new window]
Iain McDonald*
Affiliation:
Open University, Walton Hall, Kents Hill, Milton Keynes, MK7 6AA, UK email: iain.mcdonald@open.ac.uk Jodrell Bank Centre for Astrophysics, Alan Turing Building, University of Manchester, Manchester, M13 9PL, 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.

To look at propagating winds from evolved stars into the interstellar medium is to look at how they are sustained. To understand their origins, we must look to the circumstances that create them in the first instance. In this article, I examine the physical conditions under which pulsation-enhanced, dust-driven winds are first generated. These initial conditions can help constrain the late evolutionary stages of these stars and provide insight into the mechanisms that cause the mass loss itself.

Keywords

stars: AGB and post-AGBcircumstellar matterstars: fundamental parametersstars: late-typestars: mass lossstars: Population IIstars: windsoutflowsstars: variables: otherglobular clusters: general
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S366: The Origin of Outflows in Evolved Stars , November 2020 , pp. 173 - 177
Check for updates
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2022. Published by Cambridge University Press on behalf of International Astronomical Union

References

Boyer, M.L., McDonald, I., van Loon, J.Th., et al. 2009, ApJ, 705, 746 CrossRefGoogle Scholar
Boyer, M.L., van Loon, J.Th., McDonald, I., et al. 2010, ApJ, 711, L99 CrossRefGoogle Scholar
Boyer, M.L., McQuinn, K.B.W., Barmby, P., et al. 2015, ApJ, 800, 51 CrossRefGoogle Scholar
Boyer, M.L., McQuinn, K.B.W., Groenewegen, M.A.T., et al. 2017, ApJ, 851, 152 CrossRefGoogle Scholar
Cranmer, S.R., Saar, S.H. 2011, ApJ, 741, 54 CrossRefGoogle Scholar
De Beck, E., Decin, L., de Koter, A., et al. 2010, A&A, 523, 18 Google Scholar
Dupree, A.K., Hartmann, L., & Avrett, E.H. 1984, ApJ, 281, L37 CrossRefGoogle Scholar
Dupree, A.K., Smith, G.H., & Strader, J. 2009, AJ, 138, 1485 CrossRefGoogle Scholar
Gottlieb, C.A., Decin, L., Richards, A.M.S., et al. 2022, A&A, in press (arXiv:/2112.04399)Google Scholar
Handberg, R., Brogaard, K., Miglio, A., et al. 2017, MNRAS, 472, 979 CrossRefGoogle Scholar
Groenewegen, M.A.T. 2014, A&A, 561, L11 Google Scholar
McDonald, I., Boyer, M.L., Groenewegen, M.A.T., et al. 2019, MNRAS, 484, L85 CrossRefGoogle Scholar
McDonald, I., Boyer, M.L., van Loon, J.Th., et al. 2011, ApJS, 193, 23 CrossRefGoogle Scholar
McDonald, I., Boyer, M.L., van Loon, J.Th., & Sloan, G.C. 2011, ApJ, 730, 71 CrossRefGoogle Scholar
McDonald, I., De Beck, E., Lagadec, E., & Zijlstra, A.A. 2018, MNRAS, 481, 4984 CrossRefGoogle Scholar
McDonald, I., Johnson, C.I., & Zijlstra, A.A. 2011, MNRAS, 416, L6 CrossRefGoogle Scholar
McDonald, I., Sloan, G.C., Zijlstra, A.A., et al. 2010, ApJ, 717, L92 CrossRefGoogle Scholar
McDonald, I., & Trabucchi, M. 2015, MNRAS, 484, 4678 CrossRefGoogle Scholar
McDonald, I., van Loon, J.Th., Decin, L., et al. 2009, MNRAS, 394, 831 CrossRefGoogle Scholar
McDonald, I., van Loon, J.Th., Sloan, G.C., et al. 2011, MNRAS, 417, 20 CrossRefGoogle Scholar
McDonald, I., Uttenthaler, S., Zijlstra, A.A., et al. 2020, MNRAS, 491, 1174 CrossRefGoogle Scholar
McDonald, I., & Zijlstra, A.A. 2015, MNRAS, 448, 502 CrossRefGoogle Scholar
McDonald, I., Zijlstra, A.A., Sloan, G.C., et al. 2014, MNRAS, 439, 2618 CrossRefGoogle Scholar
McDonald, I., Zijlstra, A.A., Sloan, G.C., et al. 2016, MNRAS, 456, 4542 CrossRefGoogle Scholar
Miglio, A., Brogaard, K., Stello, D., et al. 2012, MNRAS, 419, 2077 CrossRefGoogle Scholar
Pastorelli, G., Marigo, P., Girardi, L., et al. 2020, MNRAS, 498, 3283 Google Scholar
Ramstedt, S., Vlemmings, W.H.T., Doan, L., et al. 2020, A&A, 640, A133 Google Scholar
Rau, G., Nielsen, K.E., Carpenter, K.G., et al. 2020, ApJ, 869, 1 CrossRefGoogle Scholar
Reimers, D. 1973, A&A, 24, 79 Google Scholar
Reimers, D. 1975, in: Baschek, B., Kegel, W.H. , & Traving, G. (eds.), Problems in stellar atmospheres and envelopes (New York: Springer–Verlag), p. 229 CrossRefGoogle Scholar
Scicluna, P., Kemper, F., McDonald, I., et al. 2022, MNRAS, 512, 1091 (arXiv:/2110.12562)CrossRefGoogle Scholar
Tailo, M., Milone, A.P., Lagioia, E.P., et al. 2020, MNRAS, 498, 5745 CrossRefGoogle Scholar
Takayama, M., Saio, H., Ita, Y. 2020, MNRAS, 431, 3189 CrossRefGoogle Scholar
van Loon, J.Th., Boyer, M.L., McDonald, I. 2008, ApJ, 680, L49 CrossRefGoogle Scholar