Low-metallicity (sub-SMC) massive stars

Bibcode
2017IAUS..329..313G
DOI
10.1017/S1743921317003088
Garcia, M.; Herrero, A.; Najarro, Francisco; Camacho, I.; Lennon, Daniel J.; Urbaneja, Miguel A.; Castro, Norberto
Bibliographical reference

The Lives and Death-Throes of Massive Stars, Proceedings of the International Astronomical Union, IAU Symposium, Volume 329, pp. 313-321

Advertised on:
11
2017
Number of authors
7
IAC number of authors
2
Citations
11
Refereed citations
9
Description
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
Non-refereed
Galaxies

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