Fig. 6

Part of the 2009 spectrum showing details of highly excited rotational lines of the TiO γ (5, 3) and (6, 4) bands. The V838 Mon spectrum (in black) is overlaid with an M5 III spectrum (in red). The latter spectrum was shifted to a heliocentric radial velocity of 88 km s-1. A narrow Hα emission line and a broad CaI absorption profile can be recognized in the spectrum of V838 Mon.
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.