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Taubenberger, S.Benetti, S.Childress, M.Pakmor, R.Hachinger, S.Mazzali, PaoloStanishev, V.Elias-Rosa, NancyAgnoletto, I.Bufano, FilomenaErgon, M.Harutyunyan, A.Inserra, C.Kankare, E.Kromer, M.Navasardyan, H.Nicolas, J.Pastorello, A.Prosperi, E.Salgado, F.Sollerman, J.Stritzinger, M.Turatto, M.Valenti, S.Hillebrandt, W.[High luminosity, slow ejecta and persistent carbon lines: SN 2009dc challenges thermonuclear explosion scenarios]

Pastorello, A.Cappellaro, E.Inserra, C.Smartt, S. J.Pignata Libralato, GiulianoBenetti, S.Valenti, S.Fraser, M.Takáts, K.Benítez Seguel, Susana AlejandraBotticella, María TeresaBrimacombe, J.Bufano, FilomenaCellier Holzem, F.Costado, M. T.Cupani, G.Curtis, I.Elias Rosa, N.Ergon, M.Fynbo, J. P.Hambsch, F. J.Hamuy Wackenhut, MarioHarutyunyan, A.Ivarson, K. M.Kankare, E.Martin, J. C.Kotak, R.LaCluyze, Aaron P.Maguire, K.Mattila, S.Maza Sancho, JoséMcCrum, M.Miluzio, M.Norgaard Nielsen, H. U.Nysewander, M. C.Ochner, P.Pan, Y. C.Pumo, M. L.Reichart, D. E.Tan, T. G.Taubenberger, S.Tomasella, L.Turatto, M.Wright, D.[INTERACTING SUPERNOVAE AND SUPERNOVA IMPOSTORS: SN 2009ip, IS THIS THE END?]

Taubenberger, S.Hachinger, S.Pignata Libralato, GiulianoMazzali, PaoloContreras, C.Valenti, S.Pastorello, A.Elias Rosa, L.Bärnbantner, O.Barwig, H.Benetti, S.Dolci, M.Fliri, J.Folatelli, GastónFreedman, W. L.González, S.Hamuy Wackenhut, MarioKrzeminski, W.Morrell, N.Navasardyan, H.Persson, S. E.Phillips, M. M.Ries, C.Roth, M.Suntzeff, Nicholas B.Turatto, M.Hillebrandt, W.[The underluminous Type Ia supernova 2005bl and the class of objects similar to SN 1991bg]

Turatto, M.Mazzali, PaoloYoung, T. R.Nomoto, K.Iwamoto, K.Benetti, S.Cappellaro, E.Danziger, I. J.Mello, D. F. dePhillips, M. M.Suntzeff, Nicholas B.Clocchiatti, A.Piemonte, A.Leibundgut, B.Covarrubias, R.Maza Sancho, JoséSollerman, J.[The peculiar type II supernova 1997D: A case for a very low Ni-56 mass]

It is well known that massive stars (M > 8 M ) evolve up to the collapse of the stellar core, resulting in most cases in a supernova (SN) explosion. Their heterogeneity is related mainly to different configurations of the progenitor star at the moment of the explosion and to their immediate envir...


Elias-Rosa, N.Van Dyk, S.D.Benetti, S.Cappellaro, E.Smith, N.Kotak, R.Turatto, M.Filippenko, A.V.Pignata, G.Fox, O.D.Galbany, L.González-Gaitán, S.Miluzio, M.Monard, L.A.G.Ergon, M.[The Type IIn Supernova SN 2010bt: The Explosion of a Star in Outburst]The Type IIn Supernova SN 2010bt: The Explosion of a Star in Outburst

Turatto, M.Clocchiatti, Alejandro.[The Peculiar Type II Supernova 1997d: a Case for a Very Low 56ni Mass1]The Peculiar Type II Supernova 1997d: a Case for a Very Low 56ni Mass1

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