First detection of a magnetic field in low-luminosity B[e] stars - New scenarios for the nature and evolutionary stages of FS CMa stars

Free Access

Table 4

Spectral fitting.

	Primary	Secondary/hot source
T_eff (K)	≤11040	≥51513
logg; g (g cm⁻²)	4.1	4.0
v_rot (km s⁻¹)	9.1	800
lr	0.57	0.43

Notes. lr is the relative contribution of bolometric fluxes of the companions to the total bolometric flux. The extreme rotation velocity of the secondary component simulates the additional hot continuum.

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.