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JWST finds the compact object in SN 1987A

Infrared integral-field spectroscopy with JWST detected narrow argon and sulphur emission lines confined to the centre of the SN 1987A remnant. Photoionisation modelling indicates the gas is being ionised either by ultraviolet and X-ray radiation from a hot cooling neutron star or by a pulsar wind nebula. After thirty-seven years in which the expected remnant had never been seen, the object the neutrino burst implied was finally located; which of the two ionisation mechanisms dominates is still argued.

Observed — measured or witnessed, with the observation cited.

Subjects

Evidence

Partly verified — Core facts are sourced; some optional detail is deliberately absent.

Recorded on Neutron star

  1. A guest star appears in Taurus and is recorded in East Asia
  2. Baade and Zwicky propose supernovae and neutron stars
  3. A regularly pulsing radio source is identified
  4. A pulsar is found inside the Crab Nebula
  5. SN 1987A: neutrinos from a collapsing core reach Earth
  6. A neutron-star merger is detected in gravitational waves and light
  7. A radius is measured for the heaviest known neutron star
  8. JWST finds the compact object in SN 1987A

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