Compact dusty clouds in cosmic environment

Abstract

A novel mechanism of the formation of compact dusty clouds in astrophysical environments is discussed. It is shown that the balance of collective forces operating in space dusty plasmas can result in the effect of dust self-confinement, generating equilibrium spherical clusters. The distribution of dust and plasma density inside such objects and their stability are investigated. Spherical dusty clouds can be formed in a broad range of plasma parameters, suggesting that this process of dust self-organization might be a generic phenomenon occurring in different astrophysical media. We argue that compact dusty clouds can represent condensation seeds for a population of small-scale, cold, gaseous clumps in the diffuse interstellar medium. They could play an important role in regulating its small-scale structure and its thermodynamical evolution.

References in corpus (2)

• Small-scale structure of the interstellar medium towards rho Oph stars: diffuse band observations
• Small-scale structure in the interstellar medium: time-varying interstellar absorption towards κ Velorum

Cited by in corpus (5)

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• Optical properties and dust temperatures in clumpy diffuse medium
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• Induced electromagnetic radiation from a charged cloud in a plane gravitational wave