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Birth of a relativistic outflow in the unusual γ-ray transient Swift J164449.3+573451
Two groups report observations of the X-ray source Swift J164449.3+573451, which was discovered when it triggered the Swift Burst Alert Telescope on 28 March 2011. Burrows et al. report that the source has increa...
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Article
A faint type of supernova from a white dwarf with a helium-rich companion
The novel properties of the faint supernova SN 2005E mean that it does not fit readily into the established supernova categories. Types Ib, Ic and II, core-collapse supernovae, are thought to form when a massi...
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Article
A γ-ray burst at a redshift of z ≈ 8.2
Two groups present redshift determinations and other spectroscopic data for the γ-ray burst GRB 090423 — now the earliest and most distant astronomical object known. Salvaterra et al. report its initial detection...
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Broadband observations of the naked-eye γ-ray burst GRB 080319B
Long-duration γ-ray bursts (GRBs) release copious amounts of energy across the entire electromagnetic spectrum, and so provide a window into the process of black hole formation from the collapse of massive sta...
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Erratum: An extremely luminous X-ray outburst at the birth of a supernova
Nature 453, 469–474 (2008) In this Article, the surname of co-author G. Bryngelson was mis-spelled as G. Byrngelson.
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An extremely luminous X-ray outburst at the birth of a supernova
Massive stars end their short lives in spectacular explosions—supernovae—that synthesize new elements and drive galaxy evolution. Historically, supernovae were discovered mainly through their ‘delayed’ optical...
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Article
An unusually brilliant transient in the galaxy M85
Many important astronomical discoveries began with the sighting of a transient light or radio source. The unusually brilliant optical transient OT2006-1, spotted in the galaxy Messier 85 in the Virgo Cluster i...
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Article
A novel explosive process is required for the γ-ray burst GRB 060614
The tidy classification system that divided γ-ray bursts (GRBs) into long-duration busts (lasting more than two seconds) and short may have had its day. The final nail in its coffin may be GRB 060614. Discover...
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Relativistic ejecta from X-ray flash XRF 060218 and the rate of cosmic explosions
A link between long γ-ray bursts (GRBs) and supernovae has been established, but whether there is a similar relationship between the weaker and softer X-ray flashes and supernovae is unclear. GRB/XRF 060218, s...
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Article
A photometric redshift of z = 6.39 ± 0.12 for GRB 050904
The γ-ray burst GRB 050904, detected by the Swift satellite on 4 September last year, is one of the most distant objects ever observed. Its redshift of z = 6.3 equates to an explosion taking place 12.8 billion ye...
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Article
The afterglow and elliptical host galaxy of the short γ-ray burst GRB 050724
Gamma-ray bursts (GRBs) are either ‘long and soft’, or ‘short and hard’. It is now clear that the long-duration type are caused by explosions of massive stars in distant star-forming galaxies. Only in recent m...
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The afterglow of GRB 050709 and the nature of the short-hard γ-ray bursts
The final chapter in the long-standing mystery of the γ-ray bursts (GRBs) centres on the origin of the short-hard class of bursts, which are suspected on theoretical grounds to result from the coalescence of n...
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Article
Kohlendioxid als Wasserstoffacceptor bei der Dehydrierung von Alkanen