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Table 1

List of sources with their stellar and accretion properties, and disk inclination when available.

Name Dist. (pc)(a) SpT(b) L (L) (b) M (M)(b) Av(b) log Lacc (L)(b) log acc (Мyr−1)(b) idisk (deg)
CVSO58 349.0 ± 2.8 K7 0.32 0.81 0.8 −1.12 −8.37 (c)
CVSO90 M0.5 0.13 0.62 0.1 −1.34 −8.61 (c)
CVSO104 M2 0.37 0.37 0.2 −1.73 −8.49 37 (c)
CVSO107 330.4 ± 2.5 M0.5 0.32 0.53 0.3 −1.30 −7.30 22.3 ± 3.9 (d)
CVSO109 400 M0.5 0.92 0.46 0.1 −0.77 −7.49 9.2 ± 2.7 (d)
CVSO146 332.0 ± 1.7 K6 0.80 0.86 0.6 −1.46 −8.57 25.8 ± 4.8 (d)
CVSO165 400 K6 0.98 0.84 0.2 −2.05 −9.10 45.85 ± 4.07 (e)
CVSO176 M3.5 0.34 0.25 1.0 −1.27 −7.84 52.4 ± 7.8 (d)

SO518 K7 0.24 0.81 1.0 −1.22 −8.53 78 (f)
SO583 385 K5 3.61 1.09 0.4 −0.30 −7.21
SO1153 K7 0.17 0.76 0.1 −0.88 −8.24 29.49

Notes. (a)Computed from Gaia EDR3 parallaxes with reliable astronometric solutions (Gaia Collaboration 2021). For those without reliable astronometric solutions (i.e. CVSO109, CVSO165 and SO583), the mean distance of the association with an uncertainty of 10% is assumed. (b)Computed in Manara et al. (2021). (c)Inclination assumed to be 60°. (d)Computed in Pittman et al. (2022) from TESS stellar rotation periods and υ sin i from Manara et al. (2021) and Kounkel et al. (2019). (e)Binary system, evidences of circumbinary disk (Frasca et al. 2021). Inclination computed as the average of the inclinations of the components. (f)Computed in Maucò et al. (in prep.).

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