pith:QPTDBMKE
JWST spectroscopy of SN 2010da/NGC 300 ULX-1: a surviving star hidden by dust
The donor star in SN 2010da has survived its outburst and returned to a heavily dust-obscured state.
arxiv:2604.13711 v2 · 2026-04-15 · astro-ph.HE
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Claims
We conclude that the donor star is likely an AGB star that has survived and is now heavily enshrouded - having returned to a dust-obscured state following a transient post-outburst phase in which the system appeared as a red supergiant.
That the radiative transfer modeling of the mid-IR SED uniquely identifies silicon carbide dust and that the measured bolometric luminosity of log(L/Lsun)=4.11 definitively indicates a surviving star rather than residual emission from other components or a failed supernova remnant.
The donor star survived the 2010 outburst, returned to a dust-obscured AGB state, and is no longer visible as a red supergiant.
Receipt and verification
| First computed | 2026-06-03T01:05:50.397698Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
83e630b144a09e414ad7e2769b52a9cbb977ae56ff22c438911632cd1be9beef
Aliases
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/QPTDBMKEUCPECSWX4J3JWUVJZO \
| 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: 83e630b144a09e414ad7e2769b52a9cbb977ae56ff22c438911632cd1be9beef
Canonical record JSON
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