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C., Marasco, A., & Fraternali, F

Intermediate-, high-velocity clouds in the Milky Way - I · 2022 · DOI 10.1093/mnras/stac987

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
open at publisher browse 2 citing papers

fields

astro-ph.GA 2

years

2026 2

verdicts

UNVERDICTED 2

representative citing papers

The origin of WHAM Point Source~46

astro-ph.GA · 2026-06-08 · unverdicted · novelty 4.0

New spectroscopy rules out PG 0931+691 as ionizer of WPS 46 and associates the source with an IVC ionized by shocks.

Modeling the Accretion of High-Velocity Clouds from a Rotating Halo

astro-ph.GA · 2026-03-30 · unverdicted · novelty 4.0

Low-angular-momentum test-particle models of HVCs originating at tens of kpc in a rotating halo reproduce observed kinematics and imply an accretion rate of several solar masses per year sufficient for long-term star formation.

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Showing 2 of 2 citing papers.

  • The origin of WHAM Point Source~46 astro-ph.GA · 2026-06-08 · unverdicted · none · ref 36

    New spectroscopy rules out PG 0931+691 as ionizer of WPS 46 and associates the source with an IVC ionized by shocks.

  • Modeling the Accretion of High-Velocity Clouds from a Rotating Halo astro-ph.GA · 2026-03-30 · unverdicted · none · ref 14

    Low-angular-momentum test-particle models of HVCs originating at tens of kpc in a rotating halo reproduce observed kinematics and imply an accretion rate of several solar masses per year sufficient for long-term star formation.