pith:HNMRHMRJ
Connecting the dusty dots: dust depletion and extinction of local interstellar clouds
Dust depletion measurements from UV spectra can be matched to peaks in 3D extinction maps to locate individual gas clouds and map metals in the local Milky Way.
arxiv:2604.24752 v2 · 2026-04-27 · astro-ph.GA
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\pithnumber{HNMRHMRJZX2ZWYHPLEAGWWXOWI}
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Claims
We show that it is possible to use complementary information from dust depletion and dust extinction to build more detailed maps of ISM metal and dust distributions.
We assume a correlation between dust depletion and dust extinction density, which we use to imply that the absorption components are spatially associated with the peaks in dust extinction density.
Dust depletion from UV spectra is associated with peaks in 3D extinction density maps to locate and chemically characterize local gas clouds at ~100 pc scales.
References
Receipt and verification
| First computed | 2026-06-03T14:05:25.136971Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3b5913b229cdf59b60ef59006b5aeeb2285029ec70e2b1b0f467f66bf03df4c1
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/HNMRHMRJZX2ZWYHPLEAGWWXOWI \
| 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: 3b5913b229cdf59b60ef59006b5aeeb2285029ec70e2b1b0f467f66bf03df4c1
Canonical record JSON
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