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How the mass-loss rates of red-supergiants determine the fate of massive stars?

Published online by Cambridge University Press:  23 May 2013

C. Georgy ,
S. Ekström ,
H. Saio ,
G. Meynet ,
J. Groh  and
A. Granada
C. Georgy
Affiliation:
CRAL, ENS-Lyon, 46 allée d’Italie, 69364 Lyon Cedex 07, France
S. Ekström
Affiliation:
Geneva Observatory, Geneva University, Chemin des Maillettes 51, 1290 Versoix, Switzerland
H. Saio
Affiliation:
Astronomical Institute, Graduate School of Science, Tohoku University, Sendai, Japan
G. Meynet
Affiliation:
Geneva Observatory, Geneva University, Chemin des Maillettes 51, 1290 Versoix, Switzerland
J. Groh
Affiliation:
Geneva Observatory, Geneva University, Chemin des Maillettes 51, 1290 Versoix, Switzerland
A. Granada
Affiliation:
Geneva Observatory, Geneva University, Chemin des Maillettes 51, 1290 Versoix, Switzerland
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Abstract

Mass-loss rates are one of the most relevant parameters determining the evolution of massive stars. In particular, the rate at which the star loses mass during the red-supergiant (RSG) phase is the least constrained by the observations or theory. In this paper, we show how the mass loss during the RSG phase affects the later evolution of the star, as well as the final type of supernova towards which it leads. We also discuss some possibilities to discriminate between blue stars that went through a RSG phase and those which remained in the blue part of the Hertzsprung-Russell diagram.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 60: Betelgeuse Workshop 2012 The Physics of Red Supergiants: Recent Advances and Open Questions , 2013 , pp. 43 - 50
Copyright
© EAS, EDP Sciences 2013

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References

Benvenuto, O.G., Bersten, M.C., & Nomoto, K., 2013, ApJ, 762, 74 CrossRef
Bersten, M.C., Benvenuto, O.G., Nomoto, K., et al., 2012, ApJ, 757, 31 CrossRef
Bresolin, F., Pietrzyński, G., Gieren, W., et al., 2004, ApJ, 600, 182 CrossRef
Chieffi, A., & Limongi, M., 2013, ApJ, 764, 21 CrossRef
Crockett, R.M., Eldridge, J.J., Smartt, S.J., et al., 2008, MNRAS, 391, L5
Crowther, P.A., 2001, ed. D. Vanbeveren, The Influence of Binaries on Stellar Population Studies, Ap&SS Library, 264, 215
de Jager, C., Nieuwenhuijzen, H., & van der Hucht, K.A., 1988, A&AS, 72, 259
Eggenberger, P., Meynet, G., Maeder, A., et al., 2008, Ap&SS, 316, 43
Ekström, S., Georgy, C., Eggenberger, P., et al., 2012, A&A, 537, A146
Elias-Rosa, N., Van Dyk, S.D., Li, W., et al., 2010, ApJ, 714, L254 CrossRef
Elias-Rosa, N., Van Dyk, S.D., Li, W., et al., 2009, ApJ, 706, 1174 CrossRef
Firnstein, M., & Przybilla, N., 2012, A&A, 543, A80
Georgy, C., 2012, A&A, 538, L8
Georgy, C., Ekström, S., Meynet, G., et al., 2012, A&A, 542, A29
Giannone, P., 1967, ZAp, 65, 226
Groh, J.H., Meynet, G., & Ekström, S., 2013, A&A, 550, L7
Humphreys, R.M., Davidson, K., Ruch, G., & Wallerstein, G., 2005, AJ, 129, 492 CrossRef
Kudritzki, R.P., Puls, J., Lennon, D.J., et al., 1999, A&A, 350, 970
Kudritzki, R.-P., Urbaneja, M.A., Bresolin, F., et al., 2008, ApJ, 681, 269 CrossRef
Levesque, E.M., Massey, P., Olsen, K.A.G., et al., 2005, ApJ, 628, 973 CrossRef
Maeder, A., & Meynet, G., 2012, Rev. Mod. Phys., 84, 25 CrossRef
Maund, J.R., Fraser, M., Ergon, M., et al., 2011, ApJ, 739, L37 CrossRef
Maund, J.R., Smartt, S.J., Kudritzki, R.P., Podsiadlowski, P., & Gilmore, G.F., 2004, Nature, 427, 129 CrossRef
Mauron, N., & Josselin, E., 2011, A&A, 526, A156
Meynet, G., & Maeder, A., 2000, A&A, 361, 101
Moriya, T., Tominaga, N., Blinnikov, S.I., Baklanov, P.V., & Sorokina, E.I., 2011, MNRAS, 415, 199 CrossRef
Podsiadlowski, P., Hsu, J.J.L., Joss, P.C., & Ross, R.R., 1993, Nature, 364, 509 CrossRef
Przybilla, N., Firnstein, M., Nieva, M.F., Meynet, G., & Maeder, A., 2010, A&A, 517, A38
Smartt, S.J., Eldridge, J.J., Crockett, R.M., & Maund, J.R., 2009, MNRAS, 395, 1409 CrossRef
Smith, N., Hinkle, K.H., & Ryde, N., 2009, AJ, 137, 3558 CrossRef
van Loon, J.T., Cioni, M.-R.L., Zijlstra, A.A., & Loup, C., 2005, A&A, 438, 273
Vanbeveren, D., De Donder, E., van Bever, J., van Rensbergen, W., & De Loore, C., 1998a, New Astron., 3, 443 CrossRef
Vanbeveren, D., De Loore, C., & Van Rensbergen, W., 1998b, A&ARv, 9, 63
Walmswell, J.J., & Eldridge, J.J., 2012, MNRAS, 419, 2054 CrossRef