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Using Spinning Dust Emission To Constrain The Abundance Of Very Small Dust Grains In Dense Cores

Tibbs, C. T. and Paladini, R. and Cleary, K. and Muchovej, S. and Scaife, A. and Stevenson, M. and Laureijs, R. and Ysard, N. and Grainge, K. and Perrott, Y. and Rumsey, C. and Villadsen, J. (2016) Using Spinning Dust Emission To Constrain The Abundance Of Very Small Dust Grains In Dense Cores. In: Conditions and impact of star formation: from lab to space : in Memory of Charles H. Townes. EAS Publications Series. No.75-76. EDP Sciences , Les Ulis, France, pp. 211-213. ISBN 978-2-7598-2022-1. http://resolver.caltech.edu/CaltechAUTHORS:20160708-081529904

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Abstract

We present the first analysis of using spinning dust emission as a method to characterise the properties of very small interstellar dust grains in dense cores.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1051/eas/1575043DOIArticle
http://www.eas-journal.org/articles/eas/abs/2015/03/eas1575043/eas1575043.htmlPublisherArticle
ORCID:
AuthorORCID
Paladini, R.0000-0002-5158-243X
Additional Information:© 2016 EAS, EDP Sciences.
Record Number:CaltechAUTHORS:20160708-081529904
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20160708-081529904
Official Citation:Using Spinning Dust Emission To Constrain The Abundance Of Very Small Dust Grains In Dense Cores C.T. Tibbs, R. Paladini, K. Cleary, S. Muchovej, A. Scaife, M. Stevenson, R. Laureijs, N. Ysard, K. Grainge, Y. Perrott, C. Rumsey and J. Villadsen EAS Publications Series, 75-76 (2015) 211-213 DOI: http://dx.doi.org/10.1051/eas/1575043
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:68908
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:09 Jul 2016 04:52
Last Modified:08 Jul 2019 21:35

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