The 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.
Primordial Resonant Lines and Observational Strategy for ODIN and HERSCHEL / MAOLI, Roberto; P., CHAMBAUD; J. Y., DANIEL; DE BERNARDIS, Paolo; P., ENCRENAZ; MASI, Silvia; B., MELCHIORRI; MELCHIORRI, Francesco; L., PAGANI; P., ROSMUS; M., SIGNORE. - In: ESA SP. - ISSN 0379-6566. - ESA SP-577:577(2005), pp. 293-296. (Intervento presentato al convegno Dusty and Molecular Universe - A prelude to HERSCHEL and ALMA tenutosi a Paris; France nel October 25-27, 2004).
Primordial Resonant Lines and Observational Strategy for ODIN and HERSCHEL
MAOLI, Roberto;DE BERNARDIS, Paolo;MASI, Silvia;MELCHIORRI, Francesco;
2005
Abstract
The 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.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
