Formation and evolution of interstellar filamentsReportar como inadecuado




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Abstract : We investigate the gas velocity dispersions of a sample of filaments recently detected as part of the Herschel Gould Belt Survey in the IC 5146, Aquila, and Polaris interstellar clouds. To measure these velocity dispersions, we use 13CO, C18O, and N2H+ line observations obtained with the IRAM 30 m telescope. Correlating our velocity dispersion measurements with the filament column densities derived from Herschel data, we show that interstellar filaments can be divided into two regimes: thermally subcritical filaments, which have transonic velocity dispersions cs ≲ σtot 



Autor: D. Arzoumanian Ph. André N. Peretto V. Könyves

Fuente: https://hal.archives-ouvertes.fr/



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