pith:L73FTK7Q
Compact HII Regions as Clocks of Massive-Star Formation: Evidence for Long Formation Timescales
Compact HII regions act as clocks showing massive stars form over Myr timescales that increase with final mass.
arxiv:2602.06196 v2 · 2026-02-05 · astro-ph.SR
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Claims
The joint LF constraints imply a growth law in which the formation time is about 4 Myr for a 60 M⊙ star, with an approximately square-root dependence on mass, as predicted by the IIM.
That the compact-HII-region phase lifetime is set solely by the time the star spends above a given ionizing luminosity while still accreting, with no significant contribution from other effects such as dust absorption or dynamical disruption of the region.
Massive stars in the Milky Way form over Myr timescales that increase with final mass, inferred from joint LF fitting of compact HII regions and OB stars under the inertial-inflow model.
References
Receipt and verification
| First computed | 2026-05-18T03:09:23.780326Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
5ff659abf066e841078b43c4b8393ad0d454eb08829a330004f64795533a8bc8
Aliases
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/L73FTK7QM3UECB4LIPCLQOJ22D \
| 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: 5ff659abf066e841078b43c4b8393ad0d454eb08829a330004f64795533a8bc8
Canonical record JSON
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