pith:SOTXRVK4
The compact neutron star in 4U 1746-37 revisited: Reassessing the mass and radius
Significant X-ray flux blocking allows the neutron star in 4U 1746-37 to match standard mass and radius values.
arxiv:2605.14264 v1 · 2026-05-14 · astro-ph.HE · astro-ph.SR
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\pithnumber{SOTXRVK4VWFKK5KWA2M3WRNMMI}
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Record completeness
Claims
Significant blocking factors (B ≳ 0.8, reducing the observed flux to ∼17% of the intrinsic emission) permit neutron star parameters consistent with the canonical values: M = 1.59 ± 0.69 M⊙, R = 13.0 ± 5.45 km, or M = 2.12 ± 1.08 M⊙, R = 9.80 ± 4.13 km.
The assumption that significant flux blocking (B ≳ 0.8) occurs and varies with photospheric radius, thereby explaining the anomalously large peak-to-touchdown flux ratio of ∼2.0.
Significant X-ray flux blocking in 4U 1746-37 allows the neutron star to have canonical mass and radius values of 1.59 solar masses and 13 km or 2.12 solar masses and 9.8 km.
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Receipt and verification
| First computed | 2026-05-17T23:39:10.455548Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
93a778d55cad8aa575560699bb45ac6212704d59a63239b6601853ca35059e5c
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/SOTXRVK4VWFKK5KWA2M3WRNMMI \
| 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: 93a778d55cad8aa575560699bb45ac6212704d59a63239b6601853ca35059e5c
Canonical record JSON
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"license": "http://creativecommons.org/licenses/by-nc-nd/4.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2026-05-14T02:08:14Z",
"title_canon_sha256": "7bcb9d11c5184035b271d8d0574acd1fde12bbf90a538865868b955ae20f394a"
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"kind": "arxiv",
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