C18O, 13CO, and 12CO abundances and excitation temperatures in the Orion B molecular cloud - Analysis of the achievable precision in modeling spectral lines within the approximation of the local thermodynamic equilibrium

Open Access

Fig. 1

Open with DEXTER Download original image

Spatial distributions of the integrated intensity (in K km s⁻¹) of the considered lines. The maps have been rotated counterclockwise by 14 degrees from the RA/Dec J2000 reference frame. The spatial offsets are given in arcsecond from the projection center located at 05^h 40^m 54.270^s, −02°28′00.00^′′. Red crosses stand for two particular lines of sight, which are analyzed in Fig. 10.

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.