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Massive stars, successes and challenges

Published online by Cambridge University Press:  28 July 2017

Georges Meynet ,
André Maeder ,
Cyril Georgy Open the ORCID record for Cyril Georgy [Opens in a new window] ,
Sylvia Ekström Open the ORCID record for Sylvia Ekström [Opens in a new window] ,
Patrick Eggenberger ,
Fabio Barblan  and
Han Feng Song
Georges Meynet
Affiliation:
Department of Astronomy, University of Geneva, Switzerland email: [email protected]
André Maeder
Affiliation:
Department of Astronomy, University of Geneva, Switzerland email: [email protected]
Cyril Georgy
Affiliation:
Department of Astronomy, University of Geneva, Switzerland email: [email protected]
Sylvia Ekström
Affiliation:
Department of Astronomy, University of Geneva, Switzerland email: [email protected]
Patrick Eggenberger
Affiliation:
Department of Astronomy, University of Geneva, Switzerland email: [email protected]
Fabio Barblan
Affiliation:
Department of Astronomy, University of Geneva, Switzerland email: [email protected]
Han Feng Song
Affiliation:
College of Science, Guizhou University, Guiyang, 550025, Guizhou Province, PR China Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650011, Kunming, PR China
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Abstract

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We give a brief overview of where we stand with respect to some old and new questions bearing on how massive stars evolve and end their lifetime. We focus on the following key points that are further discussed by other contributions during this conference: convection, mass losses, rotation, magnetic field and multiplicity. For purpose of clarity, each of these processes are discussed on its own but we have to keep in mind that they are all interacting between them offering a large variety of outputs, some of them still to be discovered.

Keywords

Massive starsconvectionmass lossrotationmagnetic fieldmultiplicity
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S329: The Lives and Death-Throes of Massive Stars , November 2016 , pp. 3 - 14
Copyright
Copyright © International Astronomical Union 2017 

References

Amorín, R., Fontana, A., Pérez-Montero, E., et al. 2017, Nature Astronomy, 1, 0052 Google Scholar
Arnett, W. D., Meakin, C., Viallet, M., et al. 2015, ApJ, 809, 30 CrossRefGoogle Scholar
Arnett, W. D. & Meakin, C., 2016, Reports on Progress in Physics, 79, 102901 Google Scholar
Beck, P. G., Montalban, J., Kallinger, T., et al. 2012, Nature, 481, 55 Google Scholar
Biermann, L., 1932, Zeitschrift für Astrophysik, 5, 117 Google Scholar
Brott, I., de Mink, S. E., Cantiello, M., et al. 2011, Astron. & Astrophys., 530, A115 CrossRefGoogle Scholar
Brüggen, M. & Hillebrandt, W., 2001, MNRAS, 320, 73 Google Scholar
Cantiello, M., Langer, N., Brott, I., et al. 2009, Astron. & Astrophys., 499, 279 CrossRefGoogle Scholar
Chiappini, C., Hirschi, R., Meynet, G., et al. 2006, Astron. & Astrophys., 449, L27 Google Scholar
Chieffi, A. & Limongi, M., 2013, ApJ, 764, 21 Google Scholar
Eggenberger, P., Lagarde, N., Miglio, A., et al. 2017, Astron. & Astrophys., 599, A18 Google Scholar
Ekström, S., Coc, A., Descouvemont, P., et al. 2010, Astron. & Astrophys., 514, A62 Google Scholar
Ekström, S., Georgy, C., Eggenberger, P., et al. 2012, Astron. & Astrophys., 537, A146 Google Scholar
Eldridge, J. J. & Stanway, E. R., 2016, MNRAS, 462, 3302 Google Scholar
Eldridge, J. J. & Stanway, E. R., 2009, MNRAS, 400, 1019 Google Scholar
Esteban, C., Mesa-Delgado, A., Morisset, C., & García-Rojas, J., 2016, MNRAS, 460, 4038 Google Scholar
Frebel, A. & Norris, J. E., 2015, Annual Review of Astronomy and Astrophysics, 53, 631 Google Scholar
Gabriel, M., Noels, A., Montalbán, J., & Miglio, A., 2014, Astron. & Astrophys., 569, A63 Google Scholar
Georgy, C., 2012, Astron. & Astrophys., 538, L8 Google Scholar
Georgy, C., Saio, H., & Meynet, G., 2014, MNRAS, 439, L6 Google Scholar
Georgy, C., Meynet, G., Ekström, S., et al. 2017, arXiv:1702.02340Google Scholar
Giannone, P., 1967, Zeitschrift für Astrophysik, 65, 226 Google Scholar
Gounelle, M., 2015, Astron. & Astrophys., 582, A26 Google Scholar
Grunhut, J. H., Wade, G. A., Neiner, C., et al. 2017, MNRAS, 465, 2432 CrossRefGoogle Scholar
Heger, A., Woosley, S. E., & Spruit, H. C., 2005, ApJ, 626, 350 Google Scholar
Humphreys, R. M., 2016, Journal of Physics Conference Series, 728, 022007 Google Scholar
Humphreys, R. M. & Martin, J. C., 2012, Eta Carinae and the Supernova Impostors, 384, 1 Google Scholar
de Jager, C., Nieuwenhuijzen, H., & van der Hucht, K. A., 1988, Astron. & Astrophys. Suppl., 72, 259 Google Scholar
de Mink, S. E., Cantiello, M., Langer, N., et al., 2009, Astron. & Astrophys., 497, 243 Google Scholar
Maeder, A. 2009, Physics, Formation and Evolution of Rotating Stars: Astronomy and Astrophysics Library. ISBN 978-3-540-76948-4. Springer Berlin Heidelberg Google Scholar
Maeder, A., Meynet, G., Ekström, S., & Georgy, C., 2009, Communications in Asteroseismology, 158, 72 Google Scholar
Maeder, A. & Meynet, G., 2012, Reviews of Modern Physics, 84, 25 Google Scholar
Martins, F., Hervé, A., Bouret, J.-C., et al. 2015, Astron. & Astrophys., 575, A34 Google Scholar
Meakin, C. A. & Arnett, D., 2007, ApJ, 667, 448 Google Scholar
Meakin, C. A. & Arnett, D., 2007, ApJ, 665, 690 CrossRefGoogle Scholar
Meynet, G., Maeder, A., Schaller, G., Schaerer, D., & Charbonnel, C. 1994, Astron. & Astrophys. Suppl., 103, 97 Google Scholar
Meynet, G., Eggenberger, P., & Maeder, A., 2011, Astron. & Astrophys., 525, L11 Google Scholar
Meynet, G., Chomienne, V., Ekström, S., et al. 2015, Astron. & Astrophys., 575, A60 CrossRefGoogle Scholar
Petit, V., Keszthelyi, Z., MacInnis, R., et al. 2017, MNRAS, 466, 1052 CrossRefGoogle Scholar
Przybilla, N., Firnstein, M., Nieva, M. F., Meynet, G., & Maeder, A., 2010, Astron. & Astrophys., 517, A38 Google Scholar
Puls, J., Vink, J. S., & Najarro, F., 2008, The Astronomy and Astrophysics Review, 16, 209 CrossRefGoogle Scholar
Salasnich, B., Bressan, A., & Chiosi, C., 1999, Astron. & Astrophys., 342, 131 Google Scholar
Sana, H., de Mink, S. E., de Koter, A., et al. 2012, Science, 337, 444 Google Scholar
Sana, H., de Koter, A., de Mink, S. E., et al. 2013, Astron. & Astrophys., 550, A107 Google Scholar
Sander, A., Hamann, W.-R., & Todt, H., 2012, Astron. & Astrophys., 540, A144 CrossRefGoogle Scholar
Smith, N., 2014, Annual Review of Astronomy and Astrophysics, 52, 487 Google Scholar
Smith, N. & Owocki, S. P., 2006, ApJL, 645, L45 Google Scholar
Song, H. F., Meynet, G., Maeder, A., Ekström, S., & Eggenberger, P., 2016, Astron. & Astrophys., 585, A120 CrossRefGoogle Scholar
Song, H. F., Maeder, A., Meynet, G., et al. 2013, Astron. & Astrophys., 556, A100 Google Scholar
Spruit, H. C., 2002, Astron. & Astrophys., 381, 923 Google Scholar
Spruit, H. C., 1999, Astron. & Astrophys., 349, 189 Google Scholar
Stanway, E. R., Eldridge, J. J., & Becker, G. D., 2016, MNRAS, 456, 485 Google Scholar
Taoso, M., Bertone, G., Meynet, G., & Ekström, S., 2008, Physical Review D, 78, 123510 CrossRefGoogle Scholar
Todini, P. & Ferrara, A., 2001, MNRAS, 325, 726 Google Scholar
Ud-Doula, A., Owocki, S. P., & Townsend, R. H. D., 2009, MNRAS, 392, 1022 Google Scholar
Ud-Doula, A., Owocki, S. P., & Townsend, R. H. D., 2008, MNRAS, 385, 97 Google Scholar
ud-Doula, A. & Owocki, S. P., 2002, ApJL, 576, 413 Google Scholar
Vanbeveren, D., Van Bever, J., & Belkus, H., 2007, ApJL, 662, L107 CrossRefGoogle Scholar
Wade, G. A., Neiner, C., Alecian, E., et al. 2016, MNRAS, 456, 2 Google Scholar
Yoon, S.-C., Dessart, L., & Clocchiatti, A. 2017, arXiv:1701.02089Google Scholar
Yoon, S.-C., Woosley, S. E., & Langer, N., 2010, ApJ, 725, 940 Google Scholar
Zahn, J.-P., 1992, Astron. & Astrophys., 265, 115 Google Scholar
Zahn, J.-P., 2011, Active OB Stars: Structure, Evolution, Mass Loss, and Critical Limits, 272, 14 Google Scholar