The morphology of the Milky Way – I. Reconstructing CO maps from simulations in fixed potentials

We present an investigation into the morphological features of the Milky Way. We use smoothed particle hydrodynamics (SPH) to simulate the interstellar medium (ISM) in the Milky Way under the effect of a number of different gravitational potentials representing spiral arms and bars, assuming that th...

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Bibliographic Details
Published inMonthly notices of the Royal Astronomical Society Vol. 444; no. 1; pp. 919 - 941
Main Authors Pettitt, Alex R., Dobbs, Clare L., Acreman, David M., Price, Daniel J.
Format Journal Article
LanguageEnglish
Published London Oxford University Press 11.10.2014
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