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Article
Open AccessJWST detection of a supernova associated with GRB 221009A without an r-process signature
Identifying the sites of r-process nucleosynthesis, a primary mechanism of heavy element production, is a key goal of astrophysics. The discovery of the brightest gamma-ray burst (GRB) to date, GRB 221009A, pr...
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Article
A kilonova following a long-duration gamma-ray burst at 350 Mpc
Gamma-ray bursts (GRBs) are divided into two populations1,2; long GRBs that derive from the core collapse of massive stars (for example, ref. 3) and short GRBs that form in the merger of two compact objects4,5. A...
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Article
An extremely energetic supernova from a very massive star in a dense medium
The interaction of a supernova with a circumstellar medium (CSM) can dramatically increase the emitted luminosity by converting kinetic energy to thermal energy. In ‘superluminous’ supernovae of type IIn—named...
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Article
The binary progenitor of Tycho Brahe's 1572 supernova
The brightness of type Ia supernovae, and their homogeneity as a class, makes them powerful tools in cosmology, yet little is known about the progenitor systems of these explosions. They are thought to arise w...
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Chapter and Conference Paper
Search for the Companions of Galactic SNe Ia
The central regions of the remnants of Galactic SNe Ia have been examined for the presence of companion stars of the exploded supernovae. We present the results of this survey for the historical SN 1572 and SN...