Pith. sign in

REVIEW 1 cited by

Three Dimensional Distribution of Atomic Hydrogen in the Milky Way

Not yet reviewed by Pith; the record is open.

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 1207.6150 v1 pith:B4HOH7NL submitted 2012-07-26 astro-ph.GA astro-ph.HEhep-ph

classification astro-ph.GAastro-ph.HEhep-ph
keywords atomicdistributionhydrogendimensionalmilkythreearmsdata
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

A new model for three dimensional distribution of atomic hydrogen gas in the Milky Way is derived using the 21cm LAB survey data. The global features of the gas distribution such as spiral arms are reproduced. The Galactic plane warps outside the solar orbit and the thickness of the gas disk flares outward the Galaxy. It is found that the mass of atomic hydrogen gas within a radius of 20 kpc is 4.3*10^9 M_Sun.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Hub-filament systems and the growth of massive stars: episodic accretion, clustered environments, and projection effects

    astro-ph.GA 2026-08 conditional novelty 6.0 of 10

    In a 3D MHD star-formation simulation, future massive stars gain about 40% of their mass in short enhanced-accretion episodes occurring preferentially near 3D hub-filament junctions, but only 27-49% of those junctions...

Pith tools