pith:LKV5HX2P
Radial Distributions of Star Formation and Gas-phase Metallicity in Spiral-Elliptical Galaxy Pairs
Spirals paired with ellipticals show suppressed central star formation and higher central metallicities.
arxiv:2604.14092 v2 · 2026-04-15 · astro-ph.GA
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Claims
Spirals in S+E pairs show suppressed central star formation and elevated metallicities, whereas spirals in spiral-spiral pairs exhibit centrally enhanced star formation and reduced metallicities; the degree depends on companion mass and gas velocity field symmetry, leading to the inference that hot CGM suppresses accretion and tidal encounters trigger enrichment.
That the observed differences in SFR and metallicity radial profiles are caused by the presence of the elliptical companion's hot circumgalactic medium and by tidal perturbations rather than by selection biases, mass differences, or other unaccounted environmental factors.
Spirals paired with ellipticals show centrally suppressed star formation and higher gas-phase metallicities than spirals paired with other spirals, with the effect scaling with companion mass and gas kinematics.
Receipt and verification
| First computed | 2026-06-19T16:09:58.178239Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
5aabd3df4f6fc26090aac341277fa4d84519c0c0bdd774692e3083aaf6e23086
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/LKV5HX2PN7BGBEFKYNASO75E3B \
| 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: 5aabd3df4f6fc26090aac341277fa4d84519c0c0bdd774692e3083aaf6e23086
Canonical record JSON
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"primary_cat": "astro-ph.GA",
"submitted_at": "2026-04-15T17:07:30Z",
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