Resolved observations at 31 GHz of spinning dust emissivity variations in ρ Oph
The ρ Oph molecular cloud is one of the best examples of spinning dust emission, first detected by the cosmic background imager (CBI). Here, we present 4.5 arcmin observations with CBI 2 that confirm 31 GHz emission from ρ Oph W, the PDR exposed to B-type star HD 147889, and highlight the absence of signal from S1, the brightest IR nebula in the
Arce-Tord, Carla et al.
Fecha de publicación:
5
2020