pith:FU64VM4F
ALMAGAL VIII. Early phases of triggered star formation in source AG286.0716$-$1.8229
Nine cores in AG286.0716-1.8229, eight aligned along an arch, show separations and masses matching the collect-and-collapse scenario of triggered star formation.
arxiv:2603.24817 v2 · 2026-03-25 · astro-ph.GA
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Claims
Comparing the typical separation and mass of the cores with those expected in the case of the collect and collapse scenario and with the thermal Jean length and mass, the best agreement is found with the characteristic scales in the case of triggered star formation.
The assumption that the adopted temperature ranges (derived from chemical tracers and dust continuum) accurately represent the cores and that the observed arch alignment is causally due to the H II region rather than projection or chance alignment.
ALMA data on nine cores along an arch in AG286.0716−1.8229 support triggered star formation induced by an expanding H II region.
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| First computed | 2026-05-27T14:06:42.428906Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
2d3dcab385c1f2e3abf505d8e7b8f1e6f3bb0d599f3f8778ba79d21129f57b80
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· · · · ·Agent API
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/FU64VM4FYHZOHK7VAXMOPOHR43 \
| 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: 2d3dcab385c1f2e3abf505d8e7b8f1e6f3bb0d599f3f8778ba79d21129f57b80
Canonical record JSON
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