pith:7VVUPXA7
RadioAstron reveals a change in the jet collimation profile of 3C 84
RadioAstron data show the jet in 3C 84 shifted from quasi-cylindrical to parabolic collimation over three years.
arxiv:2604.06803 v1 · 2026-04-08 · astro-ph.GA
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Claims
Based on measuring the collimation profile, we find that it has evolved from being quasi-cylindrical to parabolic. This is most likely the result of the decreased pressure of the mini-cocoon, which was inflated by the jet and contains hot gas that cannot confine the jet efficiently as it propagates further away from the core.
The interpretation that the observed change in collimation profile results specifically from decreased mini-cocoon pressure rather than variations in jet power, intrinsic changes in the ejection, or projection effects.
New 2016 RadioAstron observations show the jet in 3C 84 evolved from quasi-cylindrical to parabolic collimation due to decreased mini-cocoon pressure.
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Receipt and verification
| First computed | 2026-05-28T01:04:39.695311Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/7VVUPXA7WTNZIUXAYZROYGHXDG \
| jq -c '.canonical_record' \
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# expect: fd6b47dc1fb4db9452e0c662ec18f7198c6a130e3c06adf9744d73d68f328ff1
Canonical record JSON
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