Table 4: Equivalent widths of the most prominent lines detected during flare #4. A comparison is done with the classical T Tauri star LkH $_{\alpha }$ 264.
Star H $_{\alpha }$ HeI 5875 H $_{\beta }$ H $_{\gamma}$ H $_{\delta}$

V410 Tau EW(Å) at JD 2 452 238.4443 39.1 55.7 37.7

Lum. (erg s^-1) at JD 2 452 238.4443 $2.0\times10^{31}$ $2.9\times10^{31}$ $1.5\times10^{31}$

EW(Å) at JD 2 452 238.5281 27.3 3.9

Lum. (erg s^-1) at JD 2 452 238.5281 $1.4\times10^{31}$ $1.2\times10^{30}$

LkH $_{\alpha }$ 264 Average EW (Å) 94.0 2.8 29.6 16.2 11.1

**Table 4:** Equivalent widths of the most prominent lines detected during flare #4. A comparison is done with the classical T Tauri star LkH $_{\alpha }$ 264.
Star		H $_{\alpha }$	HeI 5875	H $_{\beta }$	H $_{\gamma}$	H $_{\delta}$
V410 Tau	EW(Å) at JD 2 452 238.4443			39.1	55.7	37.7
	Lum. (erg s^-1) at JD 2 452 238.4443			$2.0\times10^{31}$	$2.9\times10^{31}$	$1.5\times10^{31}$
	EW(Å) at JD 2 452 238.5281	27.3	3.9
	Lum. (erg s^-1) at JD 2 452 238.5281	$1.4\times10^{31}$	$1.2\times10^{30}$
LkH $_{\alpha }$ 264	Average EW (Å)	94.0	2.8	29.6	16.2	11.1

Source LaTeX | All tables | In the text