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Low-metallicity (sub-SMC) massive stars

Published online by Cambridge University Press:  28 July 2017

Miriam Garcia
Affiliation:
Centro de Astrobiología (INTA-CSIC), Departamento de Astrofísica. Ctra. Torrejón a Ajalvir km.4, E-28850 Torrejón de Ardoz (Madrid), Spain email: mgg@cab.inta-csic.es
Artemio Herrero
Affiliation:
Instituto de Astrofísica de Canarias, 38205 La Laguna (Tenerife), Spain Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna (Tenerife), Spain
Francisco Najarro
Affiliation:
Centro de Astrobiología (INTA-CSIC), Departamento de Astrofísica. Ctra. Torrejón a Ajalvir km.4, E-28850 Torrejón de Ardoz (Madrid), Spain email: mgg@cab.inta-csic.es
Inés Camacho
Affiliation:
Instituto de Astrofísica de Canarias, 38205 La Laguna (Tenerife), Spain Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna (Tenerife), Spain
Daniel J. Lennon
Affiliation:
European Space Astronomy Centre (ESA/ESAC), Villanueva de la Cañada (Madrid), Spain
Miguel A. Urbaneja
Affiliation:
Institut fuer Astro- und Teilchenphysik, Universitaet Innsbruck, Innsbruck, Austria
Norberto Castro
Affiliation:
Astronomy Department, University of Michigan, Ann Arbor, MI 48109, USA
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Abstract

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The double distance and metallicity frontier marked by the SMC has been finally broken with the aid of powerful multi-object spectrographs installed at 8-10m class telescopes. VLT, GTC and Keck have enabled studies of massive stars in dwarf irregular galaxies of the Local Group with poorer metal-content than the SMC. The community is working to test the predictions of evolutionary models in the low-metallicity regime, set the new standard for the metal-poor high-redshift Universe, and test the extrapolation of the physics of massive stars to environments of decreasing metallicity. In this paper, we review current knowledge on this topic.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2017 

References

Aloisi, A., Clementini, G., Tosi, M., et al. 2007, ApJL, 667, L151 Google Scholar
Azzopardi, M., Lequeux, J., & Maeder, A., 1988, A&A, 189, 34 Google Scholar
Bouret, J.-C., Lanz, T., Hillier, D. J., et al. 2015, MNRAS, 449, 1545 CrossRefGoogle Scholar
Bresolin, F., Pietrzyński, G., Urbaneja, M. A., et al. 2006, ApJ, 648, 1007 Google Scholar
Bresolin, F., Urbaneja, M. A., Gieren, W., Pietrzyński, G., & Kudritzki, R.-P., 2007, ApJ, 671, 2028 CrossRefGoogle Scholar
Brott, I., de Mink, S. E., Cantiello, M., et al. 2011a, A&A, 530, A115 Google Scholar
Camacho, I., Garcia, M., Herrero, A., & Simón-Díaz, S., 2016, A&A, 585, A82 Google Scholar
Evans, C. J., Bresolin, F., Urbaneja, M. A., et al. 2007, ApJ, 659, 1198 CrossRefGoogle Scholar
Fullerton, A. W., Massa, D. L., & Prinja, R. K., 2006, ApJ, 637, 1025 Google Scholar
Garcia, M. & Bianchi, L., 2004, ApJ, 606, 497 CrossRefGoogle Scholar
Garcia, M., Herrero, A., Castro, N., Corral, L., & Rosenberg, A., 2010, A&A, 523, A23 Google Scholar
Garcia, M. & Herrero, A., 2013, A&A, 551, A74 Google Scholar
Garcia, M., Herrero, A., Najarro, F., Lennon, D. J., & Alejandro Urbaneja, M., 2014, ApJ, 788, 64 Google Scholar
Gil de Paz, A., Gallego, J., Carrasco, E., et al., 2016, Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields, 507, 103 Google Scholar
Henault, F., Bacon, R., Bonneville, C., et al. 2003, SPIE, 4841, 1096 Google Scholar
Herrero, A., Garcia, M., Uytterhoeven, K., et al. 2010, A&A, 513, A70 Google Scholar
Herrero, A., Garcia, M., Puls, J., et al. 2012, A&A, 543, A85 Google Scholar
Hosek, M. W. Jr., Kudritzki, R.-P., Bresolin, F., et al. 2014, ApJ, 785, 151 Google Scholar
Kehrig, C., Vílchez, J. M., Pérez-Montero, E., et al. 2015, ApJL, 801, L28 Google Scholar
Kudritzki, R.-P. & Puls, J., 2000, ARA&A, 38, 613 Google Scholar
Kudritzki, R. P., 2002, ApJ, 577, 389 Google Scholar
Leitherer, C., et al., 1992, ApJ, 401, 596 Google Scholar
Leitherer, C., Leão, J. R. S., Heckman, T. M., et al. 2001, ApJ, 550, 724 Google Scholar
Lozinskaya, T. A., Arkhipova, V. P., Moiseev, A. V., & Afanas’Ev, V. L., 2002, Astronomy Reports, 46, 16 CrossRefGoogle Scholar
Madau, P. & Dickinson, M., 2014, ARA&A, 52, 415 Google Scholar
Mandel, I. & de Mink, S. E., 2016, MNRAS, 458, 2634 Google Scholar
Martins, F., Schaerer, D., & Hillier, D. J., 2005, A&A, 436, 1049 Google Scholar
Martins, F., et al., 2013, A&A, 554, A23 Google Scholar
Massey, P., Zangari, A. M., Morrell, N. I., et al. 2009, ApJ, 692, 618 CrossRefGoogle Scholar
Meynet, G., Maeder, A., Schaller, G., et al. 1994, A&AS, 103, 97 Google Scholar
Mokiem, M. R., de Koter, A., Vink, J. S., et al. 2007, A&A, 473, 603 Google Scholar
Sundqvist, J. O., Puls, J., Feldmeier, A., & Owocki, S. P., 2011, A&A, 528, A64 Google Scholar
Szécsi, D., Langer, N., Yoon, S.-C., et al. 2015, A&A, 581, A15 Google Scholar
Tautvaišienė, G., Geisler, D., Wallerstein, G., et al., 2007, AJ, 134, 2318 Google Scholar
Tramper, F., Sana, H., de Koter, A., & Kaper, L., 2011, ApJL, 741, L8 CrossRefGoogle Scholar
Tramper, F., Gräfener, G., Hartoog, O. E., et al. 2013, A&A, 559, A72 Google Scholar
Tramper, F., Sana, H., de Koter, A., Kaper, L., & Ramírez-Agudelo, O. H., 2014, A&A, 572, AA36 Google Scholar
Tramper, F., Straal, S. M., Sanyal, D., et al. 2015, A&A, 581, A110 Google Scholar
Trundle, C., Dufton, P. L., Hunter, I., et al. 2007, A&A, 471, 625 Google Scholar
Vílchez, J. M. & Iglesias-Páramo, J., 1998, ApJ, 508, 248 Google Scholar
Vink, J. S., et al., 2001, A&A, 369, 574 Google Scholar