Autor:
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.
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...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/10555
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
