PACS CH+ 3–2 lines (black, centered on the CO+ peak) overlaid on the distribution of the CO J = 6−5 peak brightness temperature (color image) observed with the CSO telescope at ~11″ resolution (Lis et al. 1998). The PACS line intensity distributions are shown in units of Jy/spaxel as a function of wavelength in μm and are not velocity resolved. White contours show the brightest regions of H–0 S (1) emission (Walmsley et al. 2000). Lower-intensity H extended emission is present in the entire field (Van der Werf et al. 1996). Violet stars show the position of the H13CN J = 1–0 clumps deeper inside the Bar (Lis & Schilke 2003).
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.