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Updated: Jan 24, 2026

Live Imaging to Study Microtubule Dynamic Instability in Taxane-resistant Breast Cancers
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Cloud Coalescence: A Dynamical Instability Affecting Multiphase Environments.

Tim Waters1, Daniel Proga2

  • 1Theoretical Division, Los Alamos National Laboratory, NM, USA.

The Astrophysical Journal. Letters
|May 21, 2019
PubMed
Summary
This summary is machine-generated.

Astrophysical clouds, even without gravity, tend to coalesce. Smaller clouds are trapped by larger ones, leading to dynamic instability and potential merging, challenging fragmentation theories.

Keywords:
galaxieshalos - galaxiesnuclei - hydrodynamics - instabilities

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Area of Science:

  • Astrophysics
  • Fluid Dynamics

Background:

  • Mass and size distributions are crucial for astrophysical objects.
  • Previous work detailed cloud formation and evolution in active galactic nuclei.
  • Large clouds were shown to exhibit damped oscillations post-formation.

Purpose of the Study:

  • Investigate interactions between astrophysical clouds of different sizes.
  • Determine the dynamic stability of cloud complexes in the absence of gravity.
  • Identify factors influencing cloud coalescence rates.

Main Methods:

  • Numerical simulations of cloud interactions.
  • Analysis of advective flows generated by larger clouds.
  • Examination of cloud response to spatial perturbations.

Main Results:

  • Smaller clouds are trapped by advective flows from larger clouds.
  • Cloud complexes are dynamically unstable without gravity.
  • Coalescence rate depends on cloud separation and transient response.
  • Turbulence can suppress coalescence.

Conclusions:

  • Cloud complexes exhibit inherent dynamic instability.
  • Coalescence is a significant factor, potentially overriding fragmentation.
  • The role of turbulence in suppressing coalescence in natural environments requires further study.