Fig. 5. Surface flux of the Ca ii...

Fig. 5.

$Surface flux of the Ca ii emission line, $F^{\prime }_{\lambda 8662}$, as a function of mass accretion rate, $\dot{M}$. The circle symbols represent the PMS stars in the molecular clouds, and the square symbols are the PMS stars in the moving groups. The open symbols show the objects with a broad Ca ii IRT emission line (FWHM > 100 km s−1), and the filled symbols represent the objects with a narrow Ca ii IRT emission line (FWHM ≤ 100 km s−1).$

Surface flux of the Ca ii emission line, |$F^{\prime }_{\lambda 8662}$|⁠, as a function of mass accretion rate, |$\dot{M}$|⁠. The circle symbols represent the PMS stars in the molecular clouds, and the square symbols are the PMS stars in the moving groups. The open symbols show the objects with a broad Ca ii IRT emission line (FWHM > 100 km s⁻¹), and the filled symbols represent the objects with a narrow Ca ii IRT emission line (FWHM ≤ 100 km s⁻¹).

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