Probing the initial conditions of high-mass star formation - IV. Gas dynamics and NH2D chemistry in high-mass precluster and protocluster clumps

Free Access

Fig. 1

Open with DEXTER Download original image

Spectra NH₂D, NH₃ (1, 1) and (2,2) overlaid with their HfS fits for the first two NH₂D cores (see Table A.2). The spectra are derived by averaging the lines within each NH₂D core scale. Other sources and spectra are presented in Fig A.1.

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.