Image Details
Caption: Figure 8.
The extended accretion flow model fit to CHIRON spectrum of CVSO 109 in Hα (left) and Hβ (right) observed on MJD = 59181.70. The observation is shown in blue. The template photosphere and chromosphere, shown as dashed orange lines, are from UVES observation of the M0 WTTS TWA 25. The light gray lines are 100 best fits, and the red lines and the dashed–dotted black lines are the average magnetospheric profiles and the total magnetosphere + chromosphere + photosphere model profiles, respectively.
© 2022. The Author(s). Published by the American Astronomical Society.