pith:OAZQTVZS
SPYGLASS. VII-B. Tracing the Fragments of Massive Star Formation Using Low-Mass Associations
Dynamical traceback links low-mass associations to shared formation sites whose feedback explains Local and Orion-Eridanus Bubble shapes.
arxiv:2604.27067 v2 · 2026-04-29 · astro-ph.GA · astro-ph.SR
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Claims
We find that feedback from the oldest co-spatial and co-moving relatives of these associations can explain the current morphologies of the Local and Orion-Eridanus Bubbles, along with the formation of related associations like Sco-Cen and Orion OB1.
The dynamical traceback accurately reconstructs past formation sites without large errors from velocity uncertainties, incomplete membership, or unaccounted gravitational interactions (invoked throughout the traceback analysis described in the abstract).
Dynamical traceback of 16 low-mass associations shows most originated from larger complexes or feedback-driven bubbles, with one possibly from an intermediate-velocity cloud collision in Orion.
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| First computed | 2026-05-20T00:01:42.309660Z |
|---|---|
| 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/OAZQTVZS3CXSGVVJP577TY7IAE \
| jq -c '.canonical_record' \
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# expect: 703309d732d8af2356a97f7ff9e3e80131314a997818872f9a931881cfe9dbf3
Canonical record JSON
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