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The reverse shock in 3D He | 1.083 um emission from fast ejecta interacting with the reverse shock (Larsson et al. 2023) Two graphs showing a blue and green ring-like structure. Two other renderings show a wireframe hourglass-shaped structure with a ring in the middle. Traces CSM between the rings — bubble-like structure instead of previously assumed hour glass or conical “walls” connecting the rings.

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The reverse shock in 3D He | 1.083 um emission from fast ejecta interacting with the reverse shock (Larsson et al. 2023) Two graphs showing a blue and green ring-like structure. Two other renderings show a wireframe hourglass-shaped structure with a ring in the middle. Traces CSM between the rings — bubble-like structure instead of previously assumed hour glass or conical “walls” connecting the rings.
https://cdn.masto.host/astrodonsocial/media_attachments/files/111/059/558/097/098/721/original/5fed7ced9810b4c7.png

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Kelly Lepo (kellylepo@astrodon.social)'s status on Friday, 15-Sep-2023 02:19:18 JST Kelly Lepo
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Ooh! The first detection of clear signals of a compact object at the center of the supernova remnant SN 1987A! It's probably either a cooling neutron star or a pulsar wind nebula.
#JWSTYearOne

In conversation about a year ago from astrodon.social permalink