The dense cores and filamentary structure of the molecular cloud in Corona Australis: Herschel SPIRE and PACS observations from the Herschel Gould Belt Survey

Free Access

Fig. A.1

Open with DEXTER Download original image

Examples of Herschel spectral energy distributions (SEDs). The upper panel shows an SED for a prestellar core, and a protostellar core SED is shown on the lower panel. The corresponding source card images are shown in Figs. A.3 and A.4, respectively.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.