Free Access

Fig. 1

image

Various 12CO transitions for Mrk 996, NGC 3353, NGC 7077, NGC 1156, and UM 448. Top row: 12CO(1–0), 12CO(2–1) (IRAM), and 12CO(2–1) (APEX) for Mrk 996; second row: 12CO(1–0) for NGC 3353 (Haro 3) for three pointings ([0, 0], [0, +10′′], [6′′, 9′′]); third row: 12CO(2–1) for NGC 3353 (Haro 3) for three pointings; fourth row: 12CO(1–0), 12CO(2–1) (IRAM), and 12CO(3–2) (APEX) for NGC 7077 (Mrk 900); fifth row: 12CO(1–0) for NGC 1156 and UM 448, and 12CO(2–1) (APEX) for UM 448; bottom row: 12CO(2–1) (IRAM) for NGC 1156 and UM 448 and 12CO(3–2) (APEX) for UM 448. The baselines are shown as a horizontal solid line, together with the multiple-component Gaussian fits as described in Sect. 3.3. The vertical axes are in units, while in Tables 2 and 3 the units are Tmb, converted from as described in Sect. 3.3. Velocity channels are as reported in Table 2. The red curves and lines refer to 30-m spectra, while the blue ones to APEX.

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.