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The Vela Pulsar and Its Pulsar Wind Nebula Vela-X Using 13 Yr of Fermi-LAT Observations

Alexander Lange et al 2025 ApJ 988 200 Long-term monitoring of the Vela pulsar finds a large Gaussian structure and a compact radial disk, both of which may be due to the pulsar’s wind; a supernova…

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Kerry Hensley7mo agoen

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Chandra Observatory reveals surprising X-ray brightness variations in supernova remnants of galaxy M83

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Faint radio signals detected from previously silent 'Blue Eye' neutron star for the first time

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Faint radio signals detected from previously silent 'Blue Eye' neutron star for the first time

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Faint radio signals detected from previously silent 'Blue Eye' neutron star for the first time

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NSF VLA Reveals Supermassive Black Holes Emit Radio "Burps" Years After Destroying Stars

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