Origin of cool cores, cold fronts and spiral structures in cool core clusters of galaxies
Hajime Inoue

TL;DR
This paper proposes a model where the movement of a brightest cluster galaxy in hot gas leads to the formation of cool cores, cold fronts, and spiral structures through gas dynamics and cooling, explaining observed features without additional heating.
Contribution
It introduces a new explanation for cool core phenomena based on galaxy motion and gas flow dynamics, without requiring extra heating mechanisms.
Findings
Reproduces observed cool cores, cold fronts, and spiral structures.
Explains suppression of cooling flows without additional heating.
Provides a dynamic model consistent with observations.
Abstract
We consider a situation in which a brightest cluster galaxy (BCG) moves in ambient hot gas in the central region of a cool core cluster of galaxies, following the study by Inoue (2014, PASJ, 66, 60). In the rest frame of the BCG, the hot gas is supposed to flow toward the BCG in parallel from a sufficiently large distance. Then, it is expected that only the gas flowing with the impact parameter less than a critical value is trapped by the gravitation field of the BCG because of the efficient radiative cooling, getting a cooling flow, and that the remaining outer gas can get over the potential well. In such a circumstance, we can draw the following picture: A boundary layer between the out-flowing gas and the trapped gas arises around the stagnation point at the back side of the BCG. Since the boundary temperature is so low as to be X-ray dim, the boundary could be observed as the cold…
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