Spectroscopy of superluminous supernova host galaxies. A preference of hydrogen-poor events for extreme emission line galaxies
Leloudas, G.; Schulze, S.; Kruehler, T.; Gorosabel, J.; Christensen, L.; Mehner, A.; Postigo, A. de Ugarte; Amorin, R.; Thoene, C. C.; Anderson, J. P.; Bauer, F. E.; Gallazzi, A.; Helminiak, K. G.; Hjorth, J.; Ibar, E.; Malesani, D.; Morrell, N.; Vinko, J.; Wheeler, J. C.;
Related identifiers: - Subject: Astrophysics - Astrophysics of Galaxiesarxiv: Astrophysics::Galaxy Astrophysics | Astrophysics::Cosmology and Extragalactic Astrophysics | Astrophysics::High Energy Astrophysical Phenomena | Astrophysics::Solar and Stellar Astrophysics
Superluminous supernovae (SLSNe) are very bright explosions that were only discovered recently and that show a preference for occurring in faint dwarf galaxies. Understanding why stellar evolution yields different types of stellar explosions in these environments is fun... View more
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Aspen Center For Physics ( ACP ) United StatesWebsite url: http://www.aspenphys.org/90%University of Szeged ( University of Szeged ) HungaryWebsite url: http://www.u-szeged.hu/90%Las Campanas Observatory ( Las Campanas Observatory ) Chile90%National Institute for Astrophysics ( INAF ) ItalyWebsite url: http://www.inaf.it/en90%Space Science Institute ( SSI ) United StatesWebsite url: http://www.spacescience.org/90%University of Szeged 90%ESRO 77%Esso Website url: http://www.esso.com/77%SPACE SCIENCE INSTITUTE 90%AGENCIA ESTATAL CONSEJO SUPERIOR DEINVESTIGACIONES CIENTIFICAS ( CSIC ) SpainWebsite url: http://www.csic.es83% - Metrics
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