High-resolution AMI Large Array imaging of spinning dust sources: spatially correlated 8 µm emission and evidence of a stellar wind in L675

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High-resolution AMI Large Array imaging of spinning dust sources: spatially correlated 8 µm emission and evidence of a stellar wind in L675

We present 25 arcsec resolution radio images of ?ve Lynds Dark Nebulae (L675, L944, L1103,L1111 and L1246) at 16 GHz made with the Arcminute Microkelvin Imager (AMI) LargeArray. These objects were previously observed with the AMI Small Array to have an excessof emission at microwave frequencies rela...

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Bibliographic Details
Main Authors:	Scaife, A., Green, D., Pooley, G., Davies, M., Franzen, Thomas, Grainge, K., Hobson, M., Hurley-Walker, Natasha, Lasenby, A., Olamaie, M., Richer, J., Rodriguez-Gonzalvez, C., Saunders, R., Scott, P., Shimwell, T., Titterington, D., Waldram, E., Zwart, J.
Format:	Journal Article
Published:	Wiley-Blackwell Publishing Ltd. 2010
Subjects:	ISM: general radiation mechanisms: general ISM: clouds stars: formation
Online Access:	http://mnrasl.oxfordjournals.org/content/403/1/L46.full.pdf+html http://hdl.handle.net/20.500.11937/33966

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