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Synthesis of the elements in stars: forty years of progressHard-X-ray emission lines from the decay of 44Ti in the remnant of supernova 1987A.Cobalt-56 γ-ray emission lines from the type Ia supernova 2014J.High-energy transients.Supernovae. ⁴⁴Ti gamma-ray emission lines from SN1987A reveal an asymmetric explosion.Gamma-ray emission from SN2014J near maximum optical lightPulsar-Driven Jets in Supernovae, Gamma-Ray Bursts, and the Universe
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Q21563903-A8A1624A-228F-4732-8194-B02ACE86BE3FQ34306725-E188A2DD-7C1C-42D4-BC19-6DE373B0ABC6Q34435553-BDAF974D-C999-4385-ADEB-1CC83210383CQ39427737-59F6CEB1-EB07-401D-BC3A-1DDD81A3FC26Q40962129-0BDAB15A-8A32-418C-8255-CDBD1150516FQ58248872-6063B241-B202-4D9A-B436-B7BB34717D5FQ58694791-B1DAD2D0-C4BF-4FA8-B464-226838F93EC6
P2860
description
article publié dans la revue scientifique Nature
@fr
scientific article published in Nature
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в Nature в лютому 1988
@uk
name
Gamma-ray line emission from SN1987A
@en
Gamma-ray line emission from SN1987A
@nl
type
label
Gamma-ray line emission from SN1987A
@en
Gamma-ray line emission from SN1987A
@nl
prefLabel
Gamma-ray line emission from SN1987A
@en
Gamma-ray line emission from SN1987A
@nl
P2093
P356
P1433
P1476
Gamma-ray line emission from SN1987A
@en
P2093
E.L. Chupp
G.H. Share
M.D. Leising
M.S. Strickman
W.R. Purcell
W.T. Vestrandt
P2888
P304
P356
10.1038/331416A0
P407
P577
1988-02-01T00:00:00Z
P6179
1045263712
P819
1988Natur.331..416M