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; J. Villadsen

doi:10.1051/eas/1575043

All issues

Volume 75-76 (2015)

EAS Publications Series, 75-76 (2015) 211-213

Abstract

Issue		EAS Publications Series Volume 75-76, 2015 Conditions and Impact of Star Formation


Page(s)		211 - 213
Section		Star Formation: Physical and Chemical Conditions, Feedback
DOI		https://doi.org/10.1051/eas/1575043
Published online		20 May 2016

Conditions and Impact of Star Formation
R. Simon, R. Schaaf and J. Stutzki (eds)
EAS Publications Series, 75–76 (2015) 211-213

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

C.T. Tibbs¹, R. Paladini², K. Cleary², S. Muchovej¹, A. Scaife³, M. Stevenson², R. Laureijs¹, N. Ysard⁴, K. Grainge³, Y. Perrott⁵, C. Rumsey⁵ and J. Villadsen¹

¹ ESA/ESTEC, Noordwijk, 2201 AZ, The Netherlands
² California Institute of Technology, Pasadena, CA 91125, USA
³ University of Manchester, Manchester, M13 9PL, UK
⁴ Université Paris-Sud, 91405 Orsay Cedex, France
⁵ University of Cambridge, Cambridge, CB3 0HE, UK

e-mail: ctibbs@cosmos.esa.int

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.