Nanoparticles designed from low pressure plasma as model for astrophysical dust clouds

Simple item page
dc.creatorStefanovic, Ilija
dc.creatorKovacevic, Eva
dc.creatorBerndt, Johannes
dc.creatorPendleton, Yvonne
dc.creatorWinter, Jorg
dc.date2004-10-13
dc.date.accessioned2026-07-07T05:52:53Z
dc.date.available2026-07-07T05:52:53Z
dc.descriptionIR spectra gained from laboratory investigations on analogue materials are an important tool for the interpretation of astronomical IR data and the understanding of the observed phenomena in DISM. Dust particles grown in argon/acetylene low pressure plasma are proposed for a new analog. We test the validity of proposed analog according to the criteria from the literature. We also present preliminary results of nitrogen band at 4.62 \$mu$m, which has been identified in dense cold dust.
dc.description12th International Congress on Plasma Physics, 25-29 October 2004, Nice (France)
dc.identifierhttps://arxiv.org/abs/physics/0410083
dc.identifierhttp://arxiv.org/abs/physics/0410083
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/86467
dc.subjectPlasma Physics
dc.titleNanoparticles designed from low pressure plasma as model for astrophysical dust clouds
dc.typetext

Files

Collections

arXiv