000002815 001__ 2815
000002815 005__ 20160701171711.0
000002815 037__ $$aASTROimport-972
000002815 100__ $$aLadjal, D.
000002815 245__ $$aHerschel PACS and SPIRE Imaging of CW Leonis
000002815 260__ $$c2011
000002815 520__ $$aFar-IR (FIR) images of the archetype carbon star CW Leo (IRC +10216)  by the Herschel Space Observatory (Pilbratt et al. 2010) reveal an extended structure at about 11' from the star which correlates with the  UV structure seen by the GALaxy Evolution EXplorer Space Observatory (GALEX) (Sahai  Chronopoulos 2010).  The UV emission is believed to be due to the  shocked asymptotic giant branch (AGB) wind with the interstellar medium  (ISM) (Sahai  Chronopoulos).  We present our main results from the Herschel data on the wind-ISM  interaction. 
000002815 700__ $$a Barlow, M.
000002815 700__ $$a Groenewegen, M.
000002815 700__ $$a Ueta, T.
000002815 700__ $$a Blommaert, J. A. D. L.
000002815 700__ $$a Cohen, M.
000002815 700__ $$a Decin, L.
000002815 700__ $$a De Meester, W.
000002815 700__ $$a Exter, K.
000002815 700__ $$a Gear, W. K.
000002815 700__ $$a Gomez, H. L.
000002815 700__ $$a Hargrave, P. C.
000002815 700__ $$a Huygen, R.
000002815 700__ $$a Ivison, R. J.
000002815 700__ $$a Jean, C.
000002815 700__ $$a Kerschbaum, F.
000002815 700__ $$a Leeks, S. J.
000002815 700__ $$a Lim, T. L.
000002815 700__ $$a Olofsson, G.
000002815 700__ $$a Polehampton, E.
000002815 700__ $$a Posch, T.
000002815 700__ $$a Regibo, S.
000002815 700__ $$a Royer, P.
000002815 700__ $$a Sibthorpe, B.
000002815 700__ $$a Swinyard, B. M.
000002815 700__ $$a Vandenbussche, B.
000002815 700__ $$a Waelkens, C.
000002815 700__ $$a Wesson, R.
000002815 773__ $$c337$$pWhy Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants$$v445$$y2011
000002815 85642 $$ahttp://esoads.eso.org/abs/2011ASPC..445..337L
000002815 905__ $$apublished in
000002815 980__ $$aNONREF