Fig. 2
22 GHz H2O maser spectrum detected toward the WF IRAS 18043−2116. The systemic velocity derived for the stellar source from the OH maser spectrum is vlsr,⋆ = 87.5 km s-1 (vertical dashed line, Deacon et al. 2004). The final spectral resolution is Δv = 0.42 km s-1, and the total velocity range covered by the maser spectral features is 400 km s-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.