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Stellar Structure and Evolution of Massive Rotating Single Stars

Published online by Cambridge University Press:  29 August 2024

R. Hirschi Open the ORCID record for R. Hirschi [Opens in a new window] ,
E. Kaiser ,
P. Eggenberger ,
S. Ekström ,
C. Georgy ,
A. Maeder  and
G. Meynet
R. Hirschi*
Affiliation:
Astrophysics Group, Lennard-Jones Laboratories, Keele University, Keele ST5 5BG, UK Kavli IPMU (WPI), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa 277-8583, Japan
E. Kaiser
Affiliation:
Astrophysics Group, Lennard-Jones Laboratories, Keele University, Keele ST5 5BG, UK
P. Eggenberger
Affiliation:
Geneva Observatory, Geneva University, CH-1290 Sauverny, Switzerland
S. Ekström
Affiliation:
Geneva Observatory, Geneva University, CH-1290 Sauverny, Switzerland
C. Georgy
Affiliation:
Geneva Observatory, Geneva University, CH-1290 Sauverny, Switzerland
A. Maeder
Affiliation:
Geneva Observatory, Geneva University, CH-1290 Sauverny, Switzerland
G. Meynet
Affiliation:
Geneva Observatory, Geneva University, CH-1290 Sauverny, Switzerland
*
email: [email protected]
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Abstract

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Rotation plays an important role in the structure and evolution of massive stars. It leads to deviation from spherical symmetry for very fast rotating stars, mixing in otherwise unmixed radiative regions and generally increased mass loss. In addition, magnetic fields interact with rotation and lead to significant transport of angular momentum. In this article, we review the various rotational and magnetic instabilities present in massive stars and their implementation in one-dimensional stellar evolution codes. We then focus on their impact on the evolution of single rotating stars. Finally, we compare rotating models to observations and discuss ways to disentangle between various uncertainties.

Keywords

rotation - hydrodynamics - magnetism - stars: evolutioninteriorsmassive
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S361: Massive Stars Near and Far , May 2022 , pp. 343 - 352
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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), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

References

Aerts, C., Mathis, S., Rogers, T. M., 2019, ARA&A, 57, 35 Google Scholar
Braithwaite, J., Spruit, H. C., 2004, Nature, 431, 819 Google Scholar
Caleo, A., Balbus, S. A., Tognelli, E., 2016, MNRAS, 460, 338 Google Scholar
Cantiello, M., Mankovich, C., Bildsten, L., Christensen-Dalsgaard, J., Paxton, B., 2014, ApJ, 788, 93 Google Scholar
Chieffi, A., Limongi, M., 2013, ApJ, 764, 21 Google Scholar
Claret, A., Torres, G., 2018, ApJ, 859, 100 Google Scholar
Cristini, A., Meakin, C., Hirschi, R., Arnett, D., Georgy, C., Viallet, M., Walkington, I., 2017, MNRAS, 471, 279 CrossRefGoogle Scholar
Deheuvels, S., et al., 2014, A&A, 564, A27 CrossRefGoogle Scholar
Edelmann, P. V. F., Röpke, F. K., Hirschi, R., Georgy, C., Jones, S., 2017, A&A, 604, A25 Google Scholar
Edelmann, P. V. F., Ratnasingam, R. P., Pedersen, M. G., Bowman, D. M., Prat, V., Rogers, T. M., 2019, ApJ, 876, 4 Google Scholar
Eggenberger, P., Meynet, G., Maeder, A., Hirschi, R., Charbonnel, C., Talon, S., Ekström, S., 2008, AP&SS, 316, 43 Google Scholar
Eggenberger, P., et al., 2019a, A&A, 621, A66 Google Scholar
Eggenberger, P., den Hartogh, J. W., Buldgen, G., Meynet, G., Salmon, S. J. A. J., Deheuvels, S., 2019b, A&A, 631, L6 CrossRefGoogle Scholar
Eggenberger, P., Buldgen, G., Salmon, S. J. A. J., Noels, A., Grevesse, N., Asplund, M., 2022, Nature Astronomy, 6, 788 Google Scholar
Ekström, S., et al., 2012, A&A, 537, A146 Google Scholar
Faucher-Giguère, C.-A., Kaspi, V. M., 2006, ApJ, 643, 332 CrossRefGoogle Scholar
Frischknecht, U., Hirschi, R., Meynet, G., Ekström, S., Georgy, C., Rauscher, T., Winteler, C., Thielemann, F. K., 2010, A&A, 522, A39 Google Scholar
Fuller, J., Ma, L., 2019, ApJL, 881, L1 CrossRefGoogle Scholar
Fuller, J., Piro, A. L., Jermyn, A. S., 2019, MNRAS, 485, 3661 Google Scholar
Gagnier, D., Rieutord, M., Charbonnel, C., Putigny, B., Espinosa Lara, F., 2019a, A&A, 625, A88 Google Scholar
Gagnier, D., Rieutord, M., Charbonnel, C., Putigny, B., Espinosa Lara, F., 2019b, A&A, 625, A89 Google Scholar
Gotthelf, E. V., Halpern, J. P., Alford, J., 2013, ApJ, 765, 58 Google Scholar
Griffiths, A., Meynet, G., Eggenberger, P., Moyano, F., Aloy, M. A., 2022, arXiv e-prints, p. arXiv:2204.00016Google Scholar
Heger, A., Langer, N., Woosley, S. E., 2000, ApJ, 528, 368 CrossRefGoogle Scholar
Heger, A., Woosley, S. E., Spruit, H. C., 2005, ApJ, 626, 350 Google Scholar
Higgins, E. R., Vink, J. S., 2019, A&A, 622, A50 Google Scholar
Hirschi, R., Maeder, A., 2010, A&A, 519, A16 Google Scholar
Hirschi, R., Meynet, G., Maeder, A., 2004, A&A, 425, 649 Google Scholar
Hirschi, R., Meynet, G., Maeder, A., 2005, A&A, 443, 581 Google Scholar
Kaiser, E., 2021, Ph.D. Thesis, Keele UniversityGoogle Scholar
Kaspi, V. M., Helfand, D. J., 2002, in Slane, P. O., Gaensler, B. M., eds, Astronomical Society of the Pacific Conference Series Vol. 271, Neutron Stars in Supernova Remnants. p. 3 (arXiv:astro-ph/0201183)Google Scholar
Langer, N., 1998, A&A, 329, 551 Google Scholar
Ma, L., Fuller, J., 2019, MNRAS, 488, 4338 Google Scholar
Maeder, A., 1997, A&A, 321, 134 Google Scholar
Maeder, A., 2009, Physics, Formation and Evolution of Rotating Stars. Springer, doi: 10.1007/978-3-540-76949-1 CrossRefGoogle Scholar
Maeder, A., Meynet, G., 2000, A&A, 361, 159 Google Scholar
Maeder, A., Meynet, G., 2005, A&A, 440, 1041 Google Scholar
Maeder, A., Zahn, J.-P., 1998, A&A, 334, 1000 Google Scholar
Marshall, F. E., Gotthelf, E. V., Zhang, W., Middleditch, J., Wang, Q. D., 1998, ApJL, 499, L179 Google Scholar
Meynet, G., Maeder, A., 1997, A&A, 321, 465 Google Scholar
Meynet, G., Maeder, A., 2002, A&A, 390, 561 Google Scholar
Muslimov, A., Page, D., 1996, ApJ, 458, 347 Google Scholar
Ogilvie, G. I., 2014, ARA&A, 52, 171 Google Scholar
Pamyatnykh, A. A., Handler, G., Dziembowski, W. A., 2004, MNRAS, 350, 1022 Google Scholar
Paxton, B., Bildsten, L., Dotter, A., Herwig, F., Lesaffre, P., Timmes, F., 2011, ApJS, 192, 3 Google Scholar
Paxton, B., et al., 2013, ApJS, 208, 4 Google Scholar
Paxton, B., et al., 2015, ApJS, 220, 15 Google Scholar
Paxton, B., et al., 2018, ApJS, 234, 34 Google Scholar
Pedersen, M. G., et al., 2021, Nature Astronomy, 5, 715 Google Scholar
Petitdemange, L., Marcotte, F., Gissinger, C., 2022, arXiv e-prints, p. arXiv:2206.13819Google Scholar
Petrovic, J., Langer, N., Yoon, S. C., Heger, A., 2005, A&A, 435, 247 Google Scholar
Popov, S. B., Turolla, R., 2012, AP&SS, 341, 457 Google Scholar
Popov, S. B., Pons, J. A., Miralles, J. A., Boldin, P. A., Posselt, B., 2010, MNRAS, 401, 2675 Google Scholar
Potter, A. T., Tout, C. A., Eldridge, J. J., 2012a, MNRAS, 419, 748 Google Scholar
Potter, A. T., Chitre, S. M., Tout, C. A., 2012b, MNRAS, 424, 2358 Google Scholar
Salmon, S. J. A. J., Moyano, F. D., Eggenberger, P., Haemmerlé, L., Buldgen, G., 2022, A&A, 664, L1Google Scholar
Spada, F., Gellert, M., Arlt, R., Deheuvels, S., 2016, A&A, 589, A23 Google Scholar
Spruit, H. C., 2002, A&A, 381, 923 Google Scholar
Talon, S., Charbonnel, C., 2005, A&A, 440, 981 Google Scholar
Talon, S., Zahn, J. P., 1997, A&A, 317, 749 Google Scholar
Tayler, R. J., 1973, MNRAS, 161, 365 Google Scholar
Varma, V., Müller, B., 2021, MNRAS, 504, 636 Google Scholar
Wheeler, J. C., Kagan, D., Chatzopoulos, E., 2015, ApJ, 799, 85 Google Scholar
Yoshida, T., Takiwaki, T., Aguilera-Dena, D. R., Kotake, K., Takahashi, K., Nakamura, K., Umeda, H., Langer, N., 2021, Monthly Notices of the Royal Astronomical Society: Letters, 506, L20Google Scholar
Zahn, J. P., 1974, in Ledoux, P., Noels, A., Rodgers, A. W., eds, IAU Symposium Vol. 59, Stellar Instability and Evolution. p. 185Google Scholar
Zahn, J. P., 1977, A&A, 57, 383 Google Scholar
Zahn, J.-P., 1992, A&A, 265, 115 Google Scholar
den Hartogh, J. W., Eggenberger, P., Hirschi, R., 2019, A&A, 622, A187 Google Scholar
den Hartogh, J. W., Eggenberger, P., Deheuvels, S., 2020, A&A, 634, L16 Google Scholar