On the nature of hydrogen-rich superluminous supernovae

Abstract We present two hydrogen-rich superluminous supernovae (SLSNe): SN2103hx and PS15br. These objects, together with SN2008es, are the only SLSNe showing a distinct, broad H α feature during the photospheric phase; also, they show no sign of strong interaction between fast moving ejecta and cir...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2018-03, Vol.475 (1), p.1046-1072
Hauptverfasser:	Inserra, C, Smartt, S J, Gall, E E E, Leloudas, G, Chen, T-W, Schulze, S, Jerkstrand, A, Nicholl, M, Anderson, J P, Arcavi, I, Benetti, S, Cartier, R A, Childress, M, Della Valle, M, Flewelling, H, Fraser, M, Gal-Yam, A, Gutiérrez, C P, Hosseinzadeh, G, Howell, D A, Huber, M, Kankare, E, Krühler, T, Magnier, E A, Maguire, K, McCully, C, Prajs, S, Primak, N, Scalzo, R, Schmidt, B P, Smith, M, Smith, K W, Tucker, B E, Valenti, S, Wilman, M, Young, D R, Yuan, F
Format:	Artikel
Sprache:	eng
Schlagworte:	Ejecta Ejection Luminosity Magnetars Photometry Photosphere Spectrophotometry Stellar evolution Strong interactions (field theory) Supernovae
Online-Zugang:	Volltext bestellen
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!