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Showing 1–3 of 3 results
Advanced filters: Author: David I. Sahman Clear advanced filters

  • 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

  • J191213.72-441045.1, the second white dwarf pulsar system found, is a binary that comprises a white dwarf in a 4.03 h orbit with an M dwarf. The system exhibits pulsed emission with a period of 5.30 min and was detected at wavelengths from radio to X-rays.

    • Ingrid Pelisoli
    • T. R. Marsh
    • J. F. Wild
    Research
    Nature Astronomy
    Volume: 7, P: 931-942

  • Parsons et al. calculate masses and radii for both members of a double white dwarf system, where the less-massive member is exhibiting non-radial g-mode pulsations, making it a prime target for asteroseismic analyses.

    • Steven G. Parsons
    • Alexander J. Brown
    • David I. Sahman
    Research
    Nature Astronomy
    Volume: 4, P: 690-696