ALMA Observations of DEM L241/LMC P3 in the Large Magellanic Cloud: Evidence for the Formation of Cool Molecular Jets Driven by a Microquasar

arXiv:2608.30489 · astro-ph.HE, astro-ph.GA · Submitted 2026-08-31 · Read on arXiv

astro-ph.HE, astro-ph.GA

Submitted: 2026-08-31

Updated: 2026-08-31

Comments: Accepted for publication in ApJL

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Alignment — 3× in this paper · explained in 1 episode
• Large Magellanic Cloud — 3× in this paper
• Abundance — 2× in this paper · explained in 1 episode
• ALMA Total Power — 1× in this paper
• Atacama Submillimeter Telescope Experiment — 1× in this paper
• Cooperation — 1× in this paper · explained in 2 episodes
• Large Velocity Gradient — 1× in this paper
• alpha — 1× in this paper · explained in 1 episode

Sources

• An ALMA view of the Jet-Arc CO clouds toward the TeV gamma-ray source HESS J1023-575 and Westerlund 2; Evidence for the footprints of microquasar jets, the very powerful cosmic-ray accelerator in the Galactic disk
• Discovery of CO Clouds Associated with the X-ray Jets of SS 433: Evidence for Shock-Cloud Interaction Enhancing Nonthermal X-ray Emission

Related papers

• Accreting Neutron Stars in Low-Mass X-ray Binaries
• Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
• Early panchromatic spectra reveal helium in the thermonuclear supernova 2024kce
• Multiwavelength Classification of Chandra Sources in Omega Centauri
• Impact of the equation of state on core collapse supernovae I: the low- T/W instability
• Secular Evolution of Quasiperiodic Eruptions: eRO-QPE2