Pith. sign in

REVIEW

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2503.17519 v1 pith:G76JCKL7 submitted 2025-03-21 astro-ph.GA

Interstellar gas motions around massive star formation regions in the nearby dwarf galaxy DDO 43

Enik\H{o} Pichler , Bendeg\'uz Koncz , Krisztina \'E. Gab\'anyi , Andr\'as P\'eter Jo\'o , L. Viktor T\'oth This is my paper
classification astro-ph.GA
keywords massiveareasdwarfenhancedformationgalaxyhydrogennearby
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

Areas of massive star formation are strongly influenced by stellar winds and supernovae, therefore, enhanced turbulent flows are expected. We analyse high-quality Karl G. Jansky Very Large Array observations of the neutral hydrogen gas content of DDO 43, a relatively nearby irregular dwarf galaxy. The line wings of neutral hydrogen spectral lines, which provide insights into local enhanced velocity dispersion, are investigated together with far-ultraviolet data, tracing emissions from massive star-forming regions. We find very weak correlations with both higher and lower velocity areas.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.