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Articles tagged: radio emission

  • Canadian Hydrogen Intensity Mapping Experiment (CHIME), Fast Radio Burst, Five-hundred meter Aperture Spherical Telescope (FAST), Lorimer burst, Survey for Tran­sient Astronomical Radio Emission 2 (STARE2) 04 November 2020 New studies reveal the origin of fast radio bursts

    ..., the Canadian Hydrogen Intensity Mapping Experiment (CHIME) and the Survey for Tran­sient Astronomical Radio Emission 2 (STARE2), in the US detected an FRB from that sky region and the event became known as FRB 200428. ...

    • Canadian Hydrogen Intensity Mapping Experiment (CHIME)
    • Fast Radio Burst
    • Five-hundred meter Aperture Spherical Telescope (FAST)
    • Lorimer burst
    • Survey for Tran­sient Astronomical Radio Emission 2 (STARE2)
  • early phase galaxy cluster merger, galaxy cluster, intercluster medium (ICM), radio emission, X-rays 12 August 2016 Astronomers spot two merging galaxy clusters bridged by X-rays

    ... reported so far, only one reported a signature of a merger shock in X-ray data and none provided concrete evidence of radio emission connected with the shocks. Therefore, this seldom observed kind of merger spotted by Akamatsu and team will...

    • early phase galaxy cluster merger
    • galaxy cluster
    • intercluster medium (ICM)
    • radio emission
    • X-rays
  • aurora, GJ 1151, LOFAR’s Two-Metre Sky Survey (LoTSS), Low-Frequency Array (LOFAR), red dwarf 17 February 2020 Earth-sized planet behind unusual star signals say astronomers

    ...the other hand lasts only for seconds or minutes at a time. This latter emission is similar to the type of emission seen in solar radio bursts. So far, most of the radio emission observed from distant stars is high frequency and it comes from a small...

    • aurora
    • GJ 1151
    • LOFAR’s Two-Metre Sky Survey (LoTSS)
    • Low-Frequency Array (LOFAR)
    • red dwarf
  • Antarctica, ARIANNA, neutrinos, Ross ice-shelf July 2017 Hunting for neutrinos in the ice of Antarctica

    .... In this charge separation, a changing current is created along the shower axis, which leads to an emissions of radio waves. In contrast to light, radio emission travel longer distances through ice before being attenuated which therefore allows for...

    • Antarctica
    • ARIANNA
    • neutrinos
    • Ross ice-shelf
    Authors: Anna Nelles    
  • B0355+54, Chandra X-ray Observatory, Geminga, pulsar wind nebulae (PWN), radio pulsar 18 January 2017 The unusual tails of a pulsar give a clue as to what type of pulse it generates

    ... Earth, conversely B0355+54 as magnetic poles directly facing the Earth. Because the radio emission occurs near the site of the magnetic poles, the radio waves may point along the direction of the jets, she said. Gamma...

    • B0355+54
    • Chandra X-ray Observatory
    • Geminga
    • pulsar wind nebulae (PWN)
    • radio pulsar
  • astrophysics, binary system, Pulsar configuration, spiral galaxy configuration April 2026 An alternative model for pulsars and spiral galaxies

    ... ‘jet’ of charged particles, at an angle to the axis of rotation, that leads to the radio emission which we observe. The angle between the spin axis and the emission cone is an assumed feature of the model. The central object in a spiral galaxy...

    • astrophysics
    • binary system
    • Pulsar configuration
    • spiral galaxy configuration
    Authors: Stuart Eves    
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