Dust-correlated cm wavelength continuum emission from translucent clouds zeta Oph and LDN 1780
Résumé
The diffuse cm wave IR-correlated signal, the 'anomalous' CMB foreground, is thought to arise in the dust in cirrus clouds. We present Cosmic Background Imager (CBI) cm wave data of two translucent clouds, zeta Oph and LDN 1780 with the aim of characterizing the anomalous emission in the translucent cloud environment.
Domaines
Astrophysique [astro-ph]Origine | Fichiers éditeurs autorisés sur une archive ouverte |
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