Spectroscopy of superluminous supernova host galaxies. A preference of hydrogen-poor events for extreme emission line galaxies
about
Gamma-ray bursts and their use as cosmic probesMass loss and stellar superwinds.Gamma-Ray Burst ProgenitorsA young stellar environment for the superluminous supernova PTF12dam★The diversity of transients from magnetar birth in core collapse supernovaeExtreme emission-line galaxies out toz~ 1 in zCOSMOSLong-rising Type II supernovae from Palomar Transient Factory and Caltech Core-Collapse ProjectMetallicity at the explosion sites of interacting transientsLow-metallicity massive single stars with rotationThe Observer’s Guide to the Gamma-Ray Burst Supernova Connection
P2860
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P2860
Spectroscopy of superluminous supernova host galaxies. A preference of hydrogen-poor events for extreme emission line galaxies
description
im März 2015 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в березні 2015
@uk
name
Spectroscopy of superluminous ...... extreme emission line galaxies
@en
Spectroscopy of superluminous ...... extreme emission line galaxies
@nl
type
label
Spectroscopy of superluminous ...... extreme emission line galaxies
@en
Spectroscopy of superluminous ...... extreme emission line galaxies
@nl
prefLabel
Spectroscopy of superluminous ...... extreme emission line galaxies
@en
Spectroscopy of superluminous ...... extreme emission line galaxies
@nl
P2093
P50
P356
P1476
Spectroscopy of superluminous ...... extreme emission line galaxies
@en
P2093
D. Malesani
F. E. Bauer
J. C. Wheeler
J. Gorosabel
J. P. Anderson
K. G. Hełminiak
N. Morrell
P304
P356
10.1093/MNRAS/STV320
P407
P50
P577
2015-03-19T00:00:00Z
P818
P819
2015MNRAS.449..917L