Literature DB >> 12144384

Supersonic turbulence and structure of interstellar molecular clouds.

Stanislav Boldyrev1, Ake Nordlund, Paolo Padoan.   

Abstract

The interstellar medium provides a unique laboratory for highly supersonic, driven hydrodynamic turbulence. We propose a theory of such turbulence, test it by numerical simulations, and use the results to explain observational scaling properties of interstellar molecular clouds, the regions where stars are born.

Year:  2002        PMID： 12144384     DOI： 10.1103/PhysRevLett.89.031102

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN： 0031-9007            Impact factor:   9.161


  1 in total

1.  Supersonic plasma turbulence in the laboratory.

Authors:  T G White; M T Oliver; P Mabey; M Kühn-Kauffeldt; A F A Bott; L N K Döhl; A R Bell; R Bingham; R Clarke; J Foster; G Giacinti; P Graham; R Heathcote; M Koenig; Y Kuramitsu; D Q Lamb; J Meinecke; Th Michel; F Miniati; M Notley; B Reville; D Ryu; S Sarkar; Y Sakawa; M P Selwood; J Squire; R H H Scott; P Tzeferacos; N Woolsey; A A Schekochihin; G Gregori
Journal:  Nat Commun       Date:  2019-04-15       Impact factor: 14.919
  1 in total

北京卡尤迪生物科技股份有限公司 © 2022-2023.