AMI radio continuum observations of young stellar objects with known outflows

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

Internet

http://hdl.handle.net/20.500.11937/5078

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