Publisher： Cambridge University Press
E-ISSN： 1743-9221|11|A29B|215-216
ISSN： 1743-9213
Source： Proceedings of the International Astronomical Union, Vol.11, Iss.A29B, 2016-10, pp. : 215-216
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
Massive stars at low metallicity are strong candidates for two of the most energetic explosions in the Universe: long duration gamma-ray bursts and superluminous supernovae. But what is the reason these explosions prefer low metallicity environments? To answer this question, we investigate how massive stellar evolution proceeds in low metallicity environments.
Related content
The role of galaxy merging in the life of massive galaxies
Proceedings of the International Astronomical Union, Vol. 11, Iss. A29B, 2016-10 ,pp. :
Access to resources
Recommend
On the origin and evolution of life in the Galaxy
International Journal of Astrobiology, Vol. 9, Iss. 4, 2010-10 ,pp. :
The nuclear path of the CNO cycles in massive stars
Proceedings of the International Astronomical Union, Vol. 11, Iss. A29B, 2016-10 ,pp. :