Star-forming regions of the Aquila rift cloud complex - II. Turbulence in molecular cores probed by NH3 emission

S. A. Levshakov; C. Henkel; D. Reimers; M. Wang

doi:10.1051/0004-6361/201423732

Home

All issues

Volume 567 (July 2014)

A&A, 567 (2014) A78

Full HTML

Free Access

Fig. A.5

Open with DEXTER Download original image

Ammonia NH₃(1, 1) and (2, 2) spectra toward the source L1251C. The channel spacing is 0.039 km s^-1; the spectral resolution FWHP = 0.045 km s^-1. The red curves show the fit of a one-component Gaussian model to the original data. The model parameters are listed in Table A.2.

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.