Fig. 7.
Download original image
Examples of fitting the SED of THA 15–31 combining the M6III with an accretion disk (and its central object) around a neutron star (top), a white dwarf (center), and a main sequence star (bottom). Details are discussed in Sect. 3.8. The arrow on the left marks the upper limit in X-rays from Swift-XRT observations. The reference distribution for the M6III is the same as that used in Fig. 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.