Pith. sign in

REVIEW 2 cited by

Dynamics of Mergers & Remnants

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 astro-ph/9811091 v1 pith:BKDK2QRO submitted 1998-11-05 astro-ph

Dynamics of Mergers & Remnants

Joshua E. Barnes This is my paper
classification astro-ph
keywords diskmergersbehaviorcoldcuspsdensitydiscussionsdynamics
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

This review focus on some issues which seem relevant to recent discussions: (1) how halo structure influences tail length, (2) the fate of power-law density cusps, (3) the results of unequal-mass disk galaxy mergers, and (4) the behavior of hot and cold gas in merging disk galaxies.

discussion (0)

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

Forward citations

Cited by 2 Pith papers

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

  1. Too many quiescent late-type galaxies or a matter of misclassification?

    astro-ph.GA 2026-07 accept novelty 6.0

    Quiescent late-type galaxies in SDSS morphological catalogues are overestimated by a factor of ~2 due to misclassified edge-on S0 galaxies.

  2. Fuelling the central region of galaxies with misaligned gas accretion

    astro-ph.GA 2026-07 conditional novelty 6.0

    Kinematically misaligned gas accretion sustains main-sequence-level star formation only below ~1e10 Msun; above that, central gas is present but dilution by pre-existing mass keeps specific star formation low.