Dust-correlated cm-wavelength continuum emission on translucent clouds ζ Oph and LDN 1780

Dust-correlated cm-wavelength continuum emission on translucent clouds ζ Oph and LDN 1780

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 characterising the anomalous emission in th...

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मुख्य लेखकों: Vidal, M, Casassus, S, Dickinson, C, Witt, A, Castellanos, P, Davies, R, Davis, R, Cabrera, G, Cleary, K, Allison, JR, Bond, JR, Bronfman, L, Bustos, R, Jones, M, Paladini, R, Pearson, T, Readhead, A, Reeves, R, Sievers, J, Taylor, A
स्वरूप: Journal article
प्रकाशित: 2011

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