most citedCan Hydrostatic Cores Form Within Isothermal Molecular Clouds?

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astro-ph2002★ 1 cited

Can Hydrostatic Cores Form Within Isothermal Molecular Clouds?

Enrique Vazquez-Semadeni, Mohsen Shadmehri, Javier Ballesteros-Paredes

Under the assumptions that molecular clouds are nearly spatially and temporally isothermal and that the density peaks (``cores'') within them are formed by turbulent fluctuations,…

astro-ph1999

Turbulent dissipation in the interstellar medium: implications for galaxy formation and evolution

V. Avila-Reese, E. Vázquez-Semadeni

We study turbulent dissipation in the ISM and explore some implications for galaxy formation and evolution using 2D MHD numerical simulations of compressible fluids. The turbulent…