Spectroscopy of superluminous supernova host galaxies. A preference of hydrogen-poor events for extreme emission line galaxies

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 fundamental in order to both unco...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2015-05, Vol.449 (1), p.917-932
Hauptverfasser:	Leloudas, G., Schulze, S., Krühler, T., Gorosabel, J., Christensen, L., Mehner, A., de Ugarte Postigo, A., Amorín, R., Thöne, C. C., Anderson, J. P., Bauer, F. E., Gallazzi, A., Hełminiak, K. G., Hjorth, J., Ibar, E., Malesani, D., Morrell, N., Vinko, J., Wheeler, J. C.
Format:	Artikel
Sprache:	eng
Schlagworte:	Dwarf galaxies Dwarf stars Emission spectroscopy Environmental conditions Explosions Galaxies Gamma ray bursts Luminosity Spectroscopy Star & galaxy formation Supernovae Supernovas
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