The lowest-metallicity type II supernova from the highest-mass red supergiant 
progenitor

Anderson, J. P.; Dessart, L.; Gutiérrez, C. P.; Krühler, T.; Galbany, L.; Jerkstrand, A.; Smartt, S. J.; Contreras, C.; Morrell, N.; Phillips, M. M.; Stritzinger, M. D.; Hsiao, E. Y.; González-Gaitán, S.; Agliozzo, C.; Castellón, S.; Chambers, K. C.; Chen, T.-W.; Flewelling, H.; Gonzalez, C.; Hosseinzadeh, G.; Huber, M.; Fraser, M.; Inserra, C.; Kankare, E.; Mattila, S.; Magnier, E.; Maguire, K.; Lowe, T. B.; Sollerman, J.; Sullivan, M.; Young, D. R.; Valenti, S.

doi:10.1038/s41550-018-0458-4

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The lowest-metallicity type II supernova from the highest-mass red supergiant progenitor

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Krühler, T.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Chen, T.-W.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Anderson, J. P., Dessart, L., Gutiérrez, C. P., Krühler, T., Galbany, L., Jerkstrand, A., et al. (2018). The lowest-metallicity type II supernova from the highest-mass red supergiant progenitor. Nature Astronomy, 2(7), 574-579. doi:10.1038/s41550-018-0458-4.

Cite as: https://hdl.handle.net/21.11116/0000-0002-5F8B-8

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