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Prevalence of neutral gas in centres of merging galaxies-II: nuclear H I, multiwavelength properties · 1908 · DOI 10.1093/mnras/stz2178

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Unveiling a cosmic tango: Integral field spectroscopy and numerical simulations of Arp 143's interaction

astro-ph.GA · 2026-06-25 · unverdicted · novelty 5.0

New spectroscopy and simulations of Arp 143 suggest it formed via head-on collision between S0 and Sc galaxies following a flyby.

Tracing Cold Gas in Absorption Across Cosmic Time with the SKA

astro-ph.GA · 2026-06-30 · unverdicted · novelty 3.0

SKAO will enable HI and OH absorption surveys to characterize cold gas properties in galaxies from z=0 to beyond z=6.

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Unveiling a cosmic tango: Integral field spectroscopy and numerical simulations of Arp 143's interaction astro-ph.GA · 2026-06-25 · unverdicted · none · ref 25
New spectroscopy and simulations of Arp 143 suggest it formed via head-on collision between S0 and Sc galaxies following a flyby.
Tracing Cold Gas in Absorption Across Cosmic Time with the SKA astro-ph.GA · 2026-06-30 · unverdicted · none · ref 154
SKAO will enable HI and OH absorption surveys to characterize cold gas properties in galaxies from z=0 to beyond z=6.

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