SIMBAD references

2019MNRAS.486..205S - Mon. Not. R. Astron. Soc., 486, 205-214 (2019/June-2)

The effect of rotation on the thermal instability of stratified galactic atmospheres - I. Local analysis.


Abstract (from CDS):

Observations show that (i) multiple gas phases can coexist in the atmospheres of galaxies and clusters; (ii) these atmospheres may be significantly rotating in the inner parts, with typical velocities that approach or even exceed the local sound speed. The thermal instability is a natural candidate to explain the formation of cold structures via condensation of a hotter gas phase. Here we systematically study the effect of rotation on the thermal stability of stratified plane-parallel atmospheres, using both analytical arguments and numerical simulations. We find that the formation of cold structures starting from small isobaric perturbations is enhanced in the regions where the rotation of the system is dynamically important (i.e. when the rotational velocity becomes comparable to the sound speed). In particular, the threshold value of the ratio between the cooling and dynamical time tcool/tdyn below which condensations can form is increased by a factor of up to ∼10 in the presence of significant rotation. We briefly discuss the implications of our results for galaxies and clusters.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): instabilities - galaxies: clusters: general - galaxies: clusters: intracluster medium - galaxies: evolution - galaxies: formation - galaxies: haloes

Status at CDS:  

Simbad objects: 4

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2019MNRAS.486..205S and select 'bookmark this link' or equivalent in the popup menu


© Université de Strasbourg/CNRS

    • Contact