pith:AI6UUN37
The Accretion Process on Protostars
Accretion onto protostars assembles most stellar mass in Class 0/I phases but lacks the unified understanding achieved for later stages.
arxiv:2605.13189 v1 · 2026-05-13 · astro-ph.SR · astro-ph.GA
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\pithnumber{AI6UUN37EUAGOJV2R7BII3FRQ2}
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Record completeness
Claims
This work aims to review recent major results, both from the observational and numerical point of view, bridging the gap between the two approaches and providing an updated, complete assessment of accretion in protostellar sources.
That recent observational and numerical results on protostellar accretion can be meaningfully compared and synthesized despite acknowledged methodological differences and caveats in parameter estimation.
The paper reviews techniques for measuring protostellar accretion, analyzes methodological differences and caveats in comparing observations with simulations, and outlines next steps for a fuller picture.
References
Receipt and verification
| First computed | 2026-05-18T03:08:56.175950Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
023d4a377f25006726ba8fc2846cb186a1ecb7d715ee3fd1112441267790806d
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/AI6UUN37EUAGOJV2R7BII3FRQ2 \
| 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: 023d4a377f25006726ba8fc2846cb186a1ecb7d715ee3fd1112441267790806d
Canonical record JSON
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"license": "http://creativecommons.org/licenses/by/4.0/",
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