Reconstructing the near- to mid-infrared environment in the stellar merger remnant V838 Monocerotis

Open Access

Fig. 25

Model we used for explaining the H-band closure phases. The red central component represents the star, while the blue ellipses may represent bipolar outflows hinted by the H band image reconstructions (cf. Figs. 23 and 24). About 95% of the model flux is contained within the central component.

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.