ASTRO On PubPhys: open In the literature: partially resolved Compiled by AI, not yet reviewed by an editor

What kind of neutron star did SN 1987A leave?

This text mentions work from 2024 on. Those parts were partly written without a live literature search and have not been checked by an editor yet.

In plain words

The 1987 supernova in a neighbouring galaxy produced a neutrino burst showing that a neutron star formed, and in 2024 JWST saw gas lit up by it, but the star itself is unseen.

Precise statement

Determine whether the compact object in SN 1987A is a cooling neutron star or powers a pulsar wind nebula, and constrain its spin and magnetic field, from the JWST-detected narrow argon lines near the center, the disputed 2021-2022 hard X-ray detections attributed to a pulsar wind nebula, and ALMA dust constraints. Answer: an identification with a luminosity budget of $\sim 10^{35}\ \text{to}\ 10^{36}\,\mathrm{erg/s}$ consistent with all bands.

What would settle it

Detection of thermal X-rays or pulsations from the center, or spatially resolved line diagnostics that discriminate a nebula from a bare cooling star.

Status in the literature

Unverified note: it names recent work and was partly written without a live literature search; it awaits a check by an editor.

2024: JWST spectra showed argon lines ionized by a central source, consistent with a neutron star but not yet distinguishing thermal emission from a pulsar wind nebula.

Revision history

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