Free Access
Fig. 4
HCN J(3–2) line at 265.886 GHz observed in comet 10P/Tempel 2 with the IRAM 30-m telescope on 10–11 July 2010. The position and relative intensities of the hyperfine components are shown and a synthetic spectrum including asymmetric outgassing (see text) and hyperfine structure is overplotted.
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.