High-resolution ALMA data identify new episodic multipolar outflow lobes in W49N showing knot chains and precession wiggles, confirming high energy and indicating conserved outflow mechanisms across stellar mass ranges.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Simulations demonstrate that YSO jet properties are controlled by stellar magnetospheric field strength and rotation, producing counter-rotating jets even from non-rotating stars and allowing upper limits on disk toroidal field from observed outflows.
citing papers explorer
-
ALMA-QUARKS view of W49N: Multipolar episodic outflow associated with the most energetic Galactic water maser
High-resolution ALMA data identify new episodic multipolar outflow lobes in W49N showing knot chains and precession wiggles, confirming high energy and indicating conserved outflow mechanisms across stellar mass ranges.
-
Modeling YSO Jets in 3D III: Dependence of Accretion and Jet Properties on Stellar Magnetospheric Field Strength and Rotation
Simulations demonstrate that YSO jet properties are controlled by stellar magnetospheric field strength and rotation, producing counter-rotating jets even from non-rotating stars and allowing upper limits on disk toroidal field from observed outflows.