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Bin-Hui Chen et al 2025 ApJ 994 124
When galactic bars form rapidly, the galaxy’s dark matter halo spin appears to have little impact, but when the process takes longer, halo spin can hasten or delay bar formation, depending on the direction of the halo’s spin.

Ricardo Yarza et al 2025 ApJL 995 L48
Long-term observations and modeling of a transient likely associated with a a star–planet merger suggest that the star was on the brink of joining the main sequence and the planet was at least several times as massive as Jupiter.

Shangjia Zhang et al 2025 ApJL 995 L33
In simulations featuring an inner disk tilted by 30 degrees, the outer disk develops a thermally driven warp due to launching of bending waves, which drives a tilting response in the outer disk.
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