Nature and evolution of the dominant carbonaceous matter in interplanetary dust particles: effects of irradiation and identification with a type of amorphous carbon

Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/33863

Title:	Nature and evolution of the dominant carbonaceous matter in interplanetary dust particles: effects of irradiation and identification with a type of amorphous carbon
Authors:	Caro,G. M. Munoz;Matrajt,G.;Dartois,E.;Nuevo,M.;d'Hendecourt,L.;Deboffle,D.;Montagnac,G.;Chauvin,N.;Boukari,C.;Le Du,D.
Contributors:	天文研究所
Keywords:	ION IRRADIATION;UV PHOTODESTRUCTION;ORGANIC-MATTER;CH BONDS;GRAINS;SPECTROSCOPY;SPECTRA;CARRIER;DISK;IR
Date:	2006
Issue Date:	2010-07-07 11:51:26 (UTC+8)
Publisher:	中央大學
Abstract:	Aims. Interplanetary dust particle (IDP) matter probably evolved under irradiation in the interstellar medium (ISM) and the solar nebula. Currently IDPs are exposed to irradiation in the Solar System. Here the effects of UV and proton processing on IDP ma
Relation:	ASTRONOMY & ASTROPHYSICS
Appears in Collections:	[Graduate Institute of Astronomy] journal & Dissertation

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