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arxiv: astro-ph/9906136 · v1 · pith:ILMZ2A5Knew · submitted 1999-06-08 · 🌌 astro-ph

TeV Measurements of Young Pulsars and Supernova Remnants

classification 🌌 astro-ph
keywords beenpulsarsremnantssupernovayoungb0540-69b1055-52detected
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Observations have been made with the University of Durham Mark 6 telescope of a number of supernova remnants and young pulsars (Vela pulsar, PSR B1055-52, PSR J1105-6107, PSR J0537-6910 and PSR B0540-69). No VHE gamma ray emission, either steady or pulsed, has been detected from these objects.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. A catalogue of TeV pulsar environments

    astro-ph.HE 2026-06 unverdicted novelty 7.0

    A homogenized catalogue of 128 TeV sources associated with 66 pulsars, covering all evolutionary stages and showing only weak correlation between luminosity and pulsar age.

  2. A catalogue of TeV pulsar environments

    astro-ph.HE 2026-06 unverdicted novelty 7.0

    A homogenized catalogue of 128 TeV sources linked to 66 pulsars shows weak correlation between TeV luminosity and pulsar age, indicating environmental effects dominate evolution.