Open Access

Fig. 5

image

Infrared spectral lines of ϵ Eridani observed with SPIRou (black points) and modelled with ZEEMAN. The wavelength of lines is shown as green vertical ticks, and the effective Landé g factors are indicated to the right of each modelled line name. The best two-component magnetic model (blue) provides an acceptable fit to all lines, while a model with no magnetic field but otherwise the same parameters (red) only fits the magnetically insensitive line (top right panel). A multi-component model (orange) provides a comparable fit to the two-component model. The observation before telluric correction (dashed line) is shown for reference.

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.