Giant stellar arcs in the Large Magellanic Cloud: a possible link with past activity of the Milky Way nucleus
Yuri N. Efremov

TL;DR
The paper proposes that the giant stellar arcs in the Large Magellanic Cloud resulted from past jet activity of the Milky Way's nucleus, which triggered star formation and created the observed arcs.
Contribution
It introduces a novel hypothesis linking the Milky Way's past activity to the formation of stellar arcs in the LMC, supported by new observational data.
Findings
Radial velocities support the jet-induced star formation hypothesis.
The arcs' orientation points toward the Milky Way's center.
Evidence suggests a past energetic jet from the Milky Way influenced the LMC.
Abstract
The origin of the giant stellar arcs in the LMC remains a controversial issue, discussed since 1966. No other stellar arc is so perfect a segment of a circle, moreover, there is another similar arc nearby. Many hypotheses were advanced to explain these arcs, and all but one of these were disproved. It was proposed in 2004 that origin of these arcs was due to the bow shock from the jet, which is intermittently fired by the Milky Way nucleus and during the last episode of its activity the jet was pointed to the LMC. Quite recently evidence for such a jet has really appeared. We suppose it was once energetic enough to trigger star formation in the LMC, and if the jet opening angle was about 2{\deg}, it could push out HI gas from the region of about 2 kpc in size, forming a cavity LMC4, but also squeezed two dense clouds, which occurred in the same area, causing the formation of stars along…
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