Torques and angular momentum: Counter-rotation in galaxies and ring galaxies
N. G. Kantharia (National Centre for Radio Astrophysics, Tata, Institute of Fundamental Research, Pune)

TL;DR
This paper proposes that gravitational torques from nearby galaxies can explain counter-rotation and ring galaxy formation, emphasizing the role of mutual gravity torques in galaxy evolution.
Contribution
It introduces a novel origin scenario where gravitational torques cause angular momentum changes, differing from traditional gas accretion or collision models.
Findings
Most counter-rotating galaxies have nearby companions within 750 kpc.
Many ring galaxies also have nearby companion galaxies.
Galaxies with close companions show significant kinematic offsets.
Abstract
We present an alternate origin scenario to explain the observed phenomena of (1) counter-rotation between different galaxy components and (2) the formation of ring galaxies. We suggest that these are direct consequences of the galaxy being acted upon by a torque which causes a change in its primordial spin angular momentum first observed as changes in the gas kinematics or distribution. We suggest that this torque is exerted by the gravitational force between nearby galaxies. This origin requires the presence of at least one companion galaxy in the vicinity - we find a companion galaxy within 750 kpc for 51/57 counter-rotating galaxies and literature indicates that all ring galaxies have a companion galaxy thus giving observable credence to this origin. Moreover in these 51 galaxies, we find a kinematic offset between stellar and gas heliocentric velocities kms for several…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astrophysics and Star Formation Studies · Stellar, planetary, and galactic studies
