Free Access

Fig. 11

thumbnail

Spectral energy distribution of two T Tauri candidates: 2XMM J223122.8+390914 (left) and 2XMM J184401.2+005455 (right). We compare the SED of the T Tauri stars with stellar atmosphere models (grey) from Castelli & Kurucz (2004) with effective temperatures 5200 K and 4000 K respectively, and log    (g) = 4.5. The optical spectra obtained at the telescope are shown as a black line, and upper limits on the magnitude are indicated with an arrow.

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.