Free Access

Fig. 2

image

Decomposition of the H2 1–0 S(1) emission in IRAS 12112+0305. Left: flux of the narrow (A) and broad (B) component of the H2 emission. Right: velocity map of the narrow (C) and broad (D) component of the H2 emission in the region where the corresponding flux is 2 × 10-18 erg s-1 cm-2 spaxel-1 for the narrow and 0.7 × 10-18 erg s-1 cm-2 spaxel-1 for the broad component. The dark contours visualize an image taken with the Hubble Space Telescope Near Infrared Camera and Multi-Object Spectrometer (HST/NICMOS) in the combined F220M+F160W+F110W filters (Scoville et al. 2000). HST contours start at ~7σ, and are drawn at 12, 19, 28, 47, 71, 95, 143, 190% of the peak intensity of the NE galaxy, which is the galaxy that shows the broad-component emission.

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.