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Showing 1–8 of 8 results
Advanced filters: Author: A. Tohuvavohu Clear advanced filters

  • The annual Fast Radio Bursts conference was again held entirely online this year, from 28 July to 5 August 2021. It included plenary talks, posters, lightning talks, late-breaking news and discussion sessions.

    • Jason W. T. Hessels
    News & Views
    Nature Astronomy
    Volume: 5, P: 1098-1099

  • The death of massive stars has traditionally been discovered by explosive events in the gamma-ray band. Liu et al. show that the sensitive wide-field monitor on board Einstein Probe can reveal a weak soft-X-ray signal much earlier than gamma rays.

    • Y. Liu
    • H. Sun
    • X.-X. Zuo
    Research
    Nature Astronomy
    Volume: 9, P: 564-576

  • A series of early-time, multiwavelength observations of an optical transient, AT2022cmc, indicate that it is a relativistic jet from a tidal disruption event originating from a supermassive black hole.

    • Igor Andreoni
    • Michael W. Coughlin
    • Jielai Zhang
    Research
    Nature
    Volume: 612, P: 430-434

  • Observations from the JWST of the second brightest GRB ever detected, GRB 230307A, indicate that it belongs to the class of long-duration GRBs resulting from compact object mergers, with the decay of lanthanides powering the longlasting optical and infrared emission.

    • Andrew J. Levan
    • Benjamin P. Gompertz
    • David Alexander Kann
    ResearchOpen Access
    Nature
    Volume: 626, P: 737-741

  • A multi-frequency observing campaign of the γ-ray burst GRB 190114C reveals a broadband double-peaked spectral energy distribution, and the teraelectronvolt emission could be attributed to inverse Compton scattering.

    • V. A. Acciari
    • S. Ansoldi
    • D. R. Young
    Research
    Nature
    Volume: 575, P: 459-463

  • Two further radio bursts associated with magnetar SGR 1935+2154 have been detected with a Westerbork 25 m dish, bringing the total to four. These observations demonstrate that SGR 1935+2154, a putative Galactic analogue of a fast radio burst source, can emit bursts across seven orders of magnitude in energy.

    • F. Kirsten
    • M. P. Snelders
    • J. Yang
    Research
    Nature Astronomy
    Volume: 5, P: 414-422