AMI radio continuum observations of young stellar objects with known outflows

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AMI radio continuum observations of young stellar objects with known outflows

We present 16 GHz (1.9 cm) deep radio continuum observations made with the Arcminute Microkelvin Imager (AMI) of a sample of low-mass young stars driving jets. We combine these new data with archival information from an extensive literature search to examine spectral energy distributions (SEDs) for...

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Bibliographic Details
Main Authors:	Ainsworth, R., Scaife, A., Ray, T., Buckle, J., Davies, M., Frantzen, T., Grainge, K., Hobson, M., Hurley-Walker, Natasha, Lasenby, A., Olamaie, M., Perrott, Y., Pooley, G., Richer, J., Rodriguez-Gonzalvez, C., Saunders, R., Schammel, M., Scott, P., Shimwell, T., Titterington, D., Waldram, E.
Format:	Journal Article
Published:	Wiley-Blackwell Publishing Ltd. 2012
Subjects:	clouds stars radiation mechanisms ISM general formation
Online Access:	http://hdl.handle.net/20.500.11937/5078

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