pith:Y6JIJ2VP
X-Shooting ULLYSES: Massive stars at low metallicity XV. On the metallicity dependence of B-supergiant mass-loss rates
B-supergiant mass-loss rates exhibit weak metallicity dependence and lack the predicted bi-stability jump, providing new empirical constraints on line-driven wind models.
arxiv:2604.21452 v2 · 2026-04-23 · astro-ph.SR
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Claims
The metallicity trends present in the mass-loss prescriptions (Z^(0.41-1.4)) explored here overestimate the empirical metallicity dependence in the B-star regime, which appears very weak. We do not find an increase in mass-loss rate at approximately spectral type B1.
That simultaneous fitting of UV and optical spectra with fastwind and Kiwi-GA yields unbiased wind parameters, including clumping factors, across the 13-29 kK temperature range without significant systematic errors from model assumptions or data quality.
B-supergiant mass-loss rates exhibit weak metallicity dependence and lack the predicted bi-stability jump, providing new empirical constraints on line-driven wind models.
Receipt and verification
| First computed | 2026-06-10T14:10:50.876845Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c79284eaaff3fc91ee825117680c0ebd3e083c484e3c44312de30073eae7a041
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/Y6JIJ2VP6P6JD3UCKELWQDAOXU \
| 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: c79284eaaff3fc91ee825117680c0ebd3e083c484e3c44312de30073eae7a041
Canonical record JSON
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