pith:EA2HHCVI
uGMRT and MeerKAT observation of RXCJ0232-4420: a quiet cluster with a giant radio halo
A cool-core galaxy cluster hosts an Mpc-scale giant radio halo sustained by minor-merger turbulence.
arxiv:2604.27123 v2 · 2026-04-29 · astro-ph.GA
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\pithnumber{EA2HHCVIUICPSVKILFDH3MZ345}
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Claims
The presence of Mpc-scale emission in the cool-core cluster shows that such emission can arise in dynamically intermediate systems. Our results demonstrate that merger-driven turbulence, even from minor disturbances, can sustain cluster-wide particle re-acceleration without destroying the cool core.
That the observed Mpc-scale radio emission is powered by merger-driven turbulence from minor disturbances rather than other mechanisms, and that the cluster's dynamical state is truly intermediate based on the survival of the cool core.
A cool-core cluster hosts a giant radio halo with uniform spectral index and sublinear radio-X-ray correlation, indicating minor-merger turbulence can sustain Mpc-scale re-acceleration without destroying the core.
Receipt and verification
| First computed | 2026-06-02T02:04:53.519542Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
2034738aa8a204f9554859467db33be76ddecab3f4b56e976334950667a57965
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/EA2HHCVIUICPSVKILFDH3MZ345 \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 2034738aa8a204f9554859467db33be76ddecab3f4b56e976334950667a57965
Canonical record JSON
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"license": "http://creativecommons.org/licenses/by-nc-nd/4.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2026-04-29T19:23:16Z",
"title_canon_sha256": "84691dcaa5ef5f3d6456723c240d410b8fcb5142cfbea38f6c77b3692c7ce720"
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