We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V star beta Pic. The disk is well resolved in the PACS filters at 70, 100, and 160 mu m. The surface brightness profiles between 70 and 160 mu m show no significant asymmetries along the disk, and are compatible with 90% of the emission between 70 and 160 mu m originating in a region closer than 200 AU to the star. Although only marginally resolving the debris disk, the maps obtained in the SPIRE 250-500 mu m filters provide full-disk photometry, completing the SED over a few octaves in wavelength that had been previously inaccessible. The small far-infrared spectral index (beta = 0.34) indicates that the grain size distribution in the inner d...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
Herschel images in six photometric bands show the thermal emission of the debris disk surrounding β ...
Context. Very few debris discs have been imaged in scattered light at wavelengths beyond 3 mum becau...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We present F435W(B), F606W (broad V), and F814W(broad I) coronagraphic images of the debris disk aro...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
Herschel images in six photometric bands show the thermal emission of the debris disk surrounding β ...
Context. Very few debris discs have been imaged in scattered light at wavelengths beyond 3 mum becau...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We present F435W(B), F606W (broad V), and F814W(broad I) coronagraphic images of the debris disk aro...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V...
Herschel images in six photometric bands show the thermal emission of the debris disk surrounding β ...
Context. Very few debris discs have been imaged in scattered light at wavelengths beyond 3 mum becau...