NettetAt z=0.01326, GRB 111005A is the third closest GRB ever detected, and second closest long duration GRB, enabling the nearby environment to be studied at a resolution of 270 pc. From the analysis of the MUSE data cube, ... Spectral analysis at the position of the GRB indicates the presence of an old stellar population ... NettetTranslations in context of "When was it launched" in English-Hebrew from Reverso Context: Tell us about the App When was it launched?
GRB 090423: probably the birth of a black hole / Credit ... - YouTube
Nettet8. jun. 2009 · Gamma-ray bursts (GRBSs) are produced by rare types of massive stellar explosions. Their rapidly fading afterglows are often bright enough at optical wavelengths, that they are detectable up to cosmological distances. Hirtheto, the highest known redshift for a GRB was z=6.7, for GRB 080913, and for a galaxy was z=6.96. Here we report … NettetPrior to the observations done on GRB 090423, the previous record holder for age and distance for GRBs was GRB 080913, which was observed in September 2008. [26] [27] … fu shing chinese
GRB 090423: Marking the Death of a Massive Star at z=8.2
NettetTerm. Grob Graphic Object Bitmap Graphics B&w Binary. File Type. GRB. Ms-dos Shell Monitor File (ms-dos 5) File Type. GRB. GARH DHRUBESWAR. Indian Railway Station. Nettet28. okt. 2009 · GRB 090423 occurred 630 million years after the Big Bang, when the Universe was only four percent of its current age of 13.7 billion years. Nettet7. apr. 2014 · CONCLUSIONS: Having identified GRB 090423 as a member of the BdHN family, we can conclude that SN events, leading to NS formation, can already occur already at z=8.2, namely at 650 Myr after the Big Bang. It is then possible that these BdHNe originate stem from 40-60 M_ {\odot} binaries. fushing name badge holders