Sourceunknownno stored text

https://arxiv.org/pdf/1710.06101

Author not recordedDate not recordedOriginal︎ ↗Archived copy

Claims1

ExaminationsNone

TextNot stored

VersionsOne known

CopiesNone recorded

CorrectionsNone recorded

Facts checked Nov 9, 2026

ReachNo copies recorded

StructureIn 1 claim's map0 sources downstream across 1 claim

EvidenceNot yet read

Examinations

None recorded. An examination is commissioned by a claim’s Steward for what its claim rests on; a review of the document for its own sake is asked for as a request bearing on it.

Text

No stored copy. Only the passages claims quote are recorded.

As quoted

X-ray absorption column densities are consistent with HI+CO-derived column densities foreground to, but not beyond, the Scutum-Crux Galactic arm, suggesting a kinematic distance of ∼3.2 kpc for HESS J1731-347.

X-ray absorption compared with CO and HI gas columns places HESS J1731-347 at least 3.2 kiloparsecs awayInconclusive

Not yet read by this claim’s Steward.

Lineage across 1 claim

Draws on · none recorded

This source

https://arxiv.org/pdf/1710.06101

in 1 claim's map

Drawn on by · none recorded

Record

Kind: unknown
Authors: Not recorded
Publisher: Not recorded
Published: Not recorded
DOI: None
Link: https://arxiv.org/pdf/1710.06101
Archived copy: https://web.archive.org/web/20251127045544/https://arxiv.org/pdf/1710.06101
Stored text: None; quoted passages only
Claims extracted: Not recorded
Versions: One known
Copies: None recorded
Corrections: None recorded
Facts checked: Nov 9, 2026

History 2

Nov 9, 2026FactsFacts fetcher · Facts looked up
Aug 5, 2026Entered the graphEntered the graph; no copy stored