Articles tagged with Hypernovae
Researchers have found evidence of a 'magneto-rotational hypernova', a previously unknown type of cataclysm that could explain the presence of high amounts of uranium and zinc in ancient stars. The discovery, published in Nature, reveals a new pathway for the formation of heavy elements in the infant universe.
A rare nearby hypernova has provided new insights into the connection between gamma-ray bursts and supernovae. Researchers discovered a hot cocoon around the jets of matter expelled by the central engine, explaining why some hypernovae do not produce GRBs.
Astronomers have detected a new component in the death of massive stars, linking gamma-ray bursts and hypernovae. The study reveals an additional hot cocoon generated around the jet, explaining differences between GRBs and hypernovae.
A supercomputer simulation demonstrates that a collapsing massive star can generate enormous magnetic fields, focusing gas along the rotation axis to create jets producing oppositely directed blasts of highly energetic gamma rays. This breakthrough model sheds light on the process behind hypernovae and gamma-ray bursts.
The ESO team has provided conclusive evidence linking cosmological gamma-ray bursts to hypernova explosions, suggesting a direct connection between the two events. The study uses unprecedented spectral data from the VLT KUEYEN telescope to determine the distance of the burst as approximately 2,650 million light-years.
The gamma ray burst, discovered by the ROTSE (Robotic Optical Transient Search Experiment) collaboration, has an intensity 100 times greater than previously observed. Its proximity to Earth allows for detailed study of its decaying light.
Astronomers have detected the first observational evidence for hypernova remnants in galaxy M101. The two remnants, MF83 and NGC5471B, are among the largest known supernova remnants and have X-ray luminosities about an order of magnitude brighter than brightest supernovae.