High luminosity, slow ejecta and persistent carbon lines: SN 2009dc challenges thermonuclear explosion scenarios

Author(s):: Taubenberger, S.; Benetti, S.; Childress, M.; Pakmor, R.; Hachinger, S.; Mazzali, P.A.; Stanishev, V.; Elias-Rosa, N.; Agnoletto, I.; Bufano, F.; Ergon, M.; Harutyunyan, A.; Inserra, C.; Kankare, E.; Kromer, M.; Navasardyan, H.; Nicolas, J.; Pastorello, A.; Prosperi, E.; Salgado Cambiazo, F.J.; Sollerman, J.; Stritzinger, M.; Turatto, M.; Valenti, S.; Hillebrandt, W.

Editor(s):: Mazzali, P. A.; Salgado, F.

Published: 2011
Publication type: Article / Letter to editor

Date issued: 2011-04-30
Language: English
Is part of: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2011), Vol. 412, no. 4, p. 2735-2762
hdl: 1887/59562
doi: 10.1111/j.1365-2966.2010.18107.x
URL: https://academic.oup.com/mnras/article/412/4/2735/1022821