2 papers
astro-ph.GA2026
A multi-scale molecular and atomic gas view on the HII region N113 in the Large Magellanic Cloud:Evidence for high-mass star formation triggered by supersonically-colliding HI flows
Rin I. Yamada, Kazuki Tokuda, Yasuo Fukui +15
The Large Magellanic Cloud (LMC) exhibits vigorous high-mass star formation, including the HII regions 30~Dor that is the most active site of star formation in the local group. The…
astro-ph.GA2025
Evidence of Galactic Interaction in the Small Magellanic Cloud Probed by Gaia Selected Massive Star Candidates
Satoya Nakano, Kengo Tachihara, Mao Tamashiro
We present identifications and kinematic analysis of 7,426 massive () stars in the Small Magellanic Cloud (SMC), using Gaia DR3 data. We used Gaia ($G_\mat…