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From the 1 of 15 linked papers with an AI index.

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15 papers

astro-ph.GA2026

Bipolar HII regions Produced by Cloud-Cloud Collisions

Theotokis Georgatos, Anthony P. Whitworth, Richard Wünsch +1

The authors run numerical simulations of head‑on collisions between 500 M⊙ clouds and show that the resulting shock‑compressed layer can produce bipolar H II regions, suggesting ma…

astro-ph.GA2026

Young star clusters in the extended UV disk of M83

M. Andersen, A. Zavagno, J. Koda +2

The process of star formation in a low-metallicity environment and whether it differs from star formation in the solar neighbourhood is an open topic. Recently, CO clumps were iden…

astro-ph.GA2026

The 10-15 GHz radio continuum survey of the Galactic Plane with SKAO

A. Traficante, C. Mininni, F. Cavallaro +63

Star formation emerges from the complex interplay between gravity, turbulence, magnetic fields, and stellar feedback, all of which vary across spatial scales and Galactic environme…

astro-ph.GA2026

The Impact and Environment of Massive Stars and Stellar Clusters

Loren Anderson, Jagadheep D. Pandian, Jyotirmoy Dey +10

Massive stars and stellar clusters shape galactic evolution through powerful feedback mechanisms including radiation pressure, photoionization, stellar winds, and cosmic ray accele…

astro-ph.GA2026

B-Fields and Star Formation across Scales with TRAO (B-FROST): CO Abundances, Dynamics and Relative Orientations in the Translucent High Latitude Cloud MBM12

J. M. Vorster, J. Montillaud, M. Juvela +14

In our Galaxy, the average star formation efficiency is of the order of a few percent. We investigated the high-latitude molecular cloud MBM12 as part of the B-fields and star form…

astro-ph.GA2026

Kinematics of the HII region NGC 7538 from study of the Ha line

D. Russeil, H. Plana, P. Amram +2

Aims. Massive stars impact their surrounding initiating star-formation along their photo-dissociation region. Once the HII region is formed it is unclear if and how the second gene…