New observations suggest that certain extremely bright supernovae are not the nuclear explosions of very massive stars. Instead, they may be ordinary-mass events lit up by a potent central fountain of magnetic energy. See Letter p.346
This is a preview of subscription content, access via your institution
Access options
References
Quimby, R. M. et al. Nature 474, 487–489 (2011).
Cooke, J. et al. Nature 491, 228–231 (2012).
Nicholl, M. et al. Nature 502, 346–349 (2013).
Barkat, Z., Rakavy, G. & Sack, N. Phys. Rev. Lett. 18, 379–381 (1967).
Gal-Yam, A. et al. Nature 462, 624–627 (2009).
Kasen, D., Woosley, S. E. & Heger, A. Astrophys. J. 734, 102 (2011).
Dessart, L., Waldman, R., Livne, E., Hillier, D. J. & Blondin, S. Mon. Not. R. Astron. Soc. 428, 3227–3251 (2013).
Kasen, D. & Bildsten, L. Astrophys. J. 717, 245–249 (2010).
Woosley, S. E. Astrophys. J. 719, L204–L207 (2010).
Maeda, K. et al. Astrophys. J. 666, 1069–1082 (2007).
Inserra, C. et al. Astrophys. J. 770, 128 (2013).
Woosley, S. E., Blinnikov, S. & Heger, A. Nature 450, 390–392 (2007).
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Kasen, D. Super-luminous supernovae on the rise. Nature 502, 310–312 (2013). https://doi.org/10.1038/502310a
Published:
Issue Date:
DOI: https://doi.org/10.1038/502310a