Abstract
The study of gas outside the plane of disc galaxies is crucial to understanding the circulation of material within a galaxy and between galaxies and the intergalactic environment. We present new HI observations of the edge-on galaxy NGC891, which show an extended halo component lagging behind the disc in rotation. We compare these results for NGC891 with other detections of gaseous haloes. Finally, we present a dynamical model for the formation of extra-planar gas.
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Fraternali, F., Oosterloo, T., Binney, J., Sancisi, R. (2007). THE GASEOUS HALOES OF DISC GALAXIES. In: DE JONG, R. (eds) ISLAND UNIVERSES. Astrophysics and Space Science Proceedings. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-5573-7_44
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DOI: https://doi.org/10.1007/978-1-4020-5573-7_44
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