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astro-ph.GA2016
A chemical solver to compute molecule and grain abundances and non-ideal MHD resistivities in prestellar core collapse calculations
Pierre Marchand, Jacques Masson, Gilles Chabrier +3
We develop a detailed chemical network relevant to the conditions characteristic of prestellar core collapse. We solve the system of time-dependent differential equations to calcul…
astro-ph.GA2016
The effect of ambipolar diffusion on low-density molecular ISM filaments
Evangelia Ntormousi, Patrick Hennebelle, Philippe André +1
The filamentary structure of the molecular interstellar medium and the potential link of this morphology to star formation have been brought into focus recently by high resolution…