pith:C3V36TPY
Deep Adaptive Optics Imaging Rules Out a Helium Star Companion to PSR J1928+1815
Deep adaptive optics imaging rules out a helium star companion to PSR J1928+1815.
arxiv:2604.03385 v2 · 2026-04-03 · astro-ph.SR · astro-ph.HE
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Claims
No source is detected at the pulsar position down to a 5σ limit of Ks ≈ 21.3. Using stripped-star atmosphere models and conservative extinction estimates, we show that any plausible helium star companion would have been detected, ruling out this interpretation.
The stripped-star atmosphere models accurately predict the near-infrared brightness for companions in the 1.0–1.6 M⊙ range, and the adopted extinction values are sufficiently conservative; if either is inaccurate, the non-detection would not fully exclude a helium star.
Deep Keck/NIRC2 adaptive optics imaging rules out a helium star companion to PSR J1928+1815, supporting a massive white dwarf with possible wind-driven eclipses.
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| First computed | 2026-06-05T00:13:46.228013Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
16ebbf4df88a23229c5e10edcf8589de5aba4713d09db4cf8314ecdb609fc622
Aliases
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/C3V36TPYRIRSFHC6CDW47BMJ3Z \
| 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())"
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Canonical record JSON
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