Abstract
The study of the physics of protostellar jets and outflows is at present significantly limited by the angular resolution and sensitivity of our telescopes. ALMA, the Atacama Large Millimeter/submillimetre Array, is under construction in northern Chile. It will provide a dramatic increase in sensitivity, resolution and spectral bandwidth at millimetre and submillimetre wavelengths compared to current facilities. I discuss the potential breakthroughs in jet science that ALMA will enable.
Cite
CITATION STYLE
Richer, J. (2009). Prospects for Outflow and Jet Science with ALMA. In Astrophysics and Space Science Proceedings (Vol. 0, pp. 429–438). Springer Science and Business Media B.V. https://doi.org/10.1007/978-3-642-00576-3_51
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