SN 2006oz: Rise of a super-luminous supernova observed by the SDSS-II SN Survey

Context. A new class of super-luminous transients has recently been identified. These objects reach absolute luminosities of Mu < -21, lack hydrogen in their spectra, and are exclusively discovered by non-targeted surveys because they are associated with very faint galaxies.

Detalhes bibliográficos
Autores: Leloudas, G., Chatzopoulos, E., Dilday, B., Gorosabel, Javier, Vinko, J., Gallazzi, A., Wheeler, J.C., Bassett, B., Fischer, J. A., Frieman, J. A., Fynbo, J. P. U., Goobar, A., Jelínek, Martin, Malesani, D., Nichol, R.C., Nordin, J., Östman, L., Sako, M., Schneider, Donald P., Smith, M., Sollerman, J., Stritzinger, M. D., Thöne, Cristina Carina, Ugarte Postigo, Antonio de
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2012
País:España
Recursos:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/422490
Acesso em linha:http://hdl.handle.net/10261/422490
Access Level:acceso abierto
Palavra-chave:Supernovae: general
Supernovae: individual: SN 2006oz
Stars: massive
Descrição
Resumo:Context. A new class of super-luminous transients has recently been identified. These objects reach absolute luminosities of Mu < -21, lack hydrogen in their spectra, and are exclusively discovered by non-targeted surveys because they are associated with very faint galaxies.

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