Table 1.

Parameters of V347 Aur used in/derived from our study.

Distance (pc)|$206.6\pm 2.3$|Gaia Collaboration (2023)
|$\log ({L_{\star }}/{{\rm L}_{\odot }})$||$-0.3\pm 0.2$|
|$T_{\rm eff}$| (K)|$3300\pm 50$|
|$\log g$| (dex)|$3.30\pm 0.10$|
|$M_{\star }$| (⁠|${\rm M}_{\odot }$|⁠)|$0.33\pm 0.05$|Baraffe et al. (2015); Feiden (2016)
|$R_{\star }$| (⁠|${\rm R}_{\odot }$|⁠)|$2.2\pm 0.3$|Baraffe et al. (2015); Feiden (2016)
Age (Myr)|$\simeq$|0.8Baraffe et al. (2015); Feiden (2016)
|$P_{\rm rot}$| (d)4.12Period used to phase data
|$P_{\rm rot}$| (d)|$4.12\pm 0.03$|From RV data
|$v \sin i$| (km s|$^{-1}$|⁠)|$12.0\pm 0.5$|From ZDI modelling
|${R_{\star }}\sin i$| (⁠|${\rm R}_{\odot }$|⁠)|$0.98\pm 0.05$|From |$R_{\star }$| and |$v \sin i$|
i (⁠|$^\circ$|⁠)|$26\pm 5$|From |$R_{\star }$| and |${R_{\star }}\sin i$|
|$r_{\rm cor}$| (au)|$0.035\pm 0.002$|From |$M_{\star }$| and |$P_{\rm rot}$|
|$r_{\rm cor}$| (⁠|$R_{\star }$|⁠)|$3.4\pm 0.6$|From |$r_{\rm cor}$| (au) and |$R_{\star }$|
|$\log {\dot{M}}$| (⁠|${\rm M}_{\odot }$| yr|$^{-1}$|⁠)|$-9.0$| to |$-6.2$|From Pa|${\beta }$| and Br|${\gamma }$|
Distance (pc)|$206.6\pm 2.3$|Gaia Collaboration (2023)
|$\log ({L_{\star }}/{{\rm L}_{\odot }})$||$-0.3\pm 0.2$|
|$T_{\rm eff}$| (K)|$3300\pm 50$|
|$\log g$| (dex)|$3.30\pm 0.10$|
|$M_{\star }$| (⁠|${\rm M}_{\odot }$|⁠)|$0.33\pm 0.05$|Baraffe et al. (2015); Feiden (2016)
|$R_{\star }$| (⁠|${\rm R}_{\odot }$|⁠)|$2.2\pm 0.3$|Baraffe et al. (2015); Feiden (2016)
Age (Myr)|$\simeq$|0.8Baraffe et al. (2015); Feiden (2016)
|$P_{\rm rot}$| (d)4.12Period used to phase data
|$P_{\rm rot}$| (d)|$4.12\pm 0.03$|From RV data
|$v \sin i$| (km s|$^{-1}$|⁠)|$12.0\pm 0.5$|From ZDI modelling
|${R_{\star }}\sin i$| (⁠|${\rm R}_{\odot }$|⁠)|$0.98\pm 0.05$|From |$R_{\star }$| and |$v \sin i$|
i (⁠|$^\circ$|⁠)|$26\pm 5$|From |$R_{\star }$| and |${R_{\star }}\sin i$|
|$r_{\rm cor}$| (au)|$0.035\pm 0.002$|From |$M_{\star }$| and |$P_{\rm rot}$|
|$r_{\rm cor}$| (⁠|$R_{\star }$|⁠)|$3.4\pm 0.6$|From |$r_{\rm cor}$| (au) and |$R_{\star }$|
|$\log {\dot{M}}$| (⁠|${\rm M}_{\odot }$| yr|$^{-1}$|⁠)|$-9.0$| to |$-6.2$|From Pa|${\beta }$| and Br|${\gamma }$|
Table 1.

Parameters of V347 Aur used in/derived from our study.

Distance (pc)|$206.6\pm 2.3$|Gaia Collaboration (2023)
|$\log ({L_{\star }}/{{\rm L}_{\odot }})$||$-0.3\pm 0.2$|
|$T_{\rm eff}$| (K)|$3300\pm 50$|
|$\log g$| (dex)|$3.30\pm 0.10$|
|$M_{\star }$| (⁠|${\rm M}_{\odot }$|⁠)|$0.33\pm 0.05$|Baraffe et al. (2015); Feiden (2016)
|$R_{\star }$| (⁠|${\rm R}_{\odot }$|⁠)|$2.2\pm 0.3$|Baraffe et al. (2015); Feiden (2016)
Age (Myr)|$\simeq$|0.8Baraffe et al. (2015); Feiden (2016)
|$P_{\rm rot}$| (d)4.12Period used to phase data
|$P_{\rm rot}$| (d)|$4.12\pm 0.03$|From RV data
|$v \sin i$| (km s|$^{-1}$|⁠)|$12.0\pm 0.5$|From ZDI modelling
|${R_{\star }}\sin i$| (⁠|${\rm R}_{\odot }$|⁠)|$0.98\pm 0.05$|From |$R_{\star }$| and |$v \sin i$|
i (⁠|$^\circ$|⁠)|$26\pm 5$|From |$R_{\star }$| and |${R_{\star }}\sin i$|
|$r_{\rm cor}$| (au)|$0.035\pm 0.002$|From |$M_{\star }$| and |$P_{\rm rot}$|
|$r_{\rm cor}$| (⁠|$R_{\star }$|⁠)|$3.4\pm 0.6$|From |$r_{\rm cor}$| (au) and |$R_{\star }$|
|$\log {\dot{M}}$| (⁠|${\rm M}_{\odot }$| yr|$^{-1}$|⁠)|$-9.0$| to |$-6.2$|From Pa|${\beta }$| and Br|${\gamma }$|
Distance (pc)|$206.6\pm 2.3$|Gaia Collaboration (2023)
|$\log ({L_{\star }}/{{\rm L}_{\odot }})$||$-0.3\pm 0.2$|
|$T_{\rm eff}$| (K)|$3300\pm 50$|
|$\log g$| (dex)|$3.30\pm 0.10$|
|$M_{\star }$| (⁠|${\rm M}_{\odot }$|⁠)|$0.33\pm 0.05$|Baraffe et al. (2015); Feiden (2016)
|$R_{\star }$| (⁠|${\rm R}_{\odot }$|⁠)|$2.2\pm 0.3$|Baraffe et al. (2015); Feiden (2016)
Age (Myr)|$\simeq$|0.8Baraffe et al. (2015); Feiden (2016)
|$P_{\rm rot}$| (d)4.12Period used to phase data
|$P_{\rm rot}$| (d)|$4.12\pm 0.03$|From RV data
|$v \sin i$| (km s|$^{-1}$|⁠)|$12.0\pm 0.5$|From ZDI modelling
|${R_{\star }}\sin i$| (⁠|${\rm R}_{\odot }$|⁠)|$0.98\pm 0.05$|From |$R_{\star }$| and |$v \sin i$|
i (⁠|$^\circ$|⁠)|$26\pm 5$|From |$R_{\star }$| and |${R_{\star }}\sin i$|
|$r_{\rm cor}$| (au)|$0.035\pm 0.002$|From |$M_{\star }$| and |$P_{\rm rot}$|
|$r_{\rm cor}$| (⁠|$R_{\star }$|⁠)|$3.4\pm 0.6$|From |$r_{\rm cor}$| (au) and |$R_{\star }$|
|$\log {\dot{M}}$| (⁠|${\rm M}_{\odot }$| yr|$^{-1}$|⁠)|$-9.0$| to |$-6.2$|From Pa|${\beta }$| and Br|${\gamma }$|
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