Primordial Resonant Lines and Observational Strategy for ODIN and HERSCHEL

Simple item page
dc.creatorMaoli, R.
dc.creatorChambaud, P.
dc.creatorDaniel, J. Y.
dc.creatorde Bernardis, P.
dc.creatorEncrenaz, P.
dc.creatorMasi, S.
dc.creatorMelchiorri, B.
dc.creatorMelchiorri, F.
dc.creatorPagani, L.
dc.creatorRosmus, P.
dc.creatorSignore, M.
dc.date2004-11-23
dc.date.accessioned2026-07-07T02:15:59Z
dc.date.available2026-07-07T02:15:59Z
dc.descriptionThe presence of a primordial molecular or atomic medium can give us the possibility to investigate the first phases of the structure formation. The lines produced by resonant scattering of the CMB photons are the most important signals coming from the dark age of the post-recombination universe. The possibility to detect these lines with ODIN and Herschel satellites are investigated.
dc.description4 pages; to appear in ESA SP-577, Proceedings of the conference "Dusty and Molecular Universe - A prelude to HERSCHEL and ALMA", October 25-27, 2004, Paris
dc.identifierhttps://arxiv.org/abs/astro-ph/0411641
dc.identifierhttp://arxiv.org/abs/astro-ph/0411641
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8619
dc.subjectAstrophysics
dc.titlePrimordial Resonant Lines and Observational Strategy for ODIN and HERSCHEL
dc.typetext

Files

Collections

arXiv