Using more than 15 years of observations from the Parkes radio telescope, astronomers detected three rotational glitches in the pulsar PSR J1637−4642—a young neutron star that had shown no signs of glitches since its discovery. The three glitches included one that changed its rotation rate by nearly 3 parts per million. Their paper was posted to the arXiv preprint server on Aug. 20. It has been accepted for publication in the Astrophysical Journal Letters.
Astronomers Detect Three Glitches in Young Neutron Star PSR J1637−4642
Astronomers using the Parkes radio telescope observed three glitches in the pulsar PSR J1637−4642, a young neutron star that had previously shown no glitches. This discovery, documented in a paper accepted for publication in the Astrophysical Journal Letters, highlights new findings in astrophysics but does not have direct implications for Iran.
📰 What Happened
Astronomers detected three glitches in the pulsar PSR J1637−4642, a young neutron star, using observations from the Parkes radio telescope. This discovery is significant as it marks the first time glitches have been observed in this pulsar since its discovery.
- The glitches included a change in rotation rate by nearly 3 parts per million.
- The findings were documented in a paper accepted for publication in the Astrophysical Journal Letters.
💡 Why It Matters
📚 Background
Neutron stars are remnants of massive stars that have undergone supernova explosions, and glitches in their rotation can provide insights into their internal structure and behavior.
🏷️ Entities Mentioned
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