Table 1: Characteristic values for the VLTP, for various MTS values. Note the dispersion in born again times according to the adopted MTS value. The third column shows characteristic time for the duration of the peak of proton burning. The born-again times correspond to the time interval from the moment of maximum $T_{\rm eff}$ after the H burning (and at high luminosity) until $\log{T_{\rm eff}}=3.8$ is reached for the first time.
MTS $\int{L{\rm _H dt}}$ [erg] $\Delta t$ [days] Born-again

$L_{\rm H}>(e^{-1} \times {L_{\rm H}}_{\rm max} )$ time-scale [yr]

$1\times 10^{-5}$ $4.5\times 10^{47}$ 0.113 8.7

$3\times 10^{-5}$ $4.31\times 10^{47}$ 0.133 10.3

$1\times 10^{-4}$ $3.75\times 10^{47}$ 0.209 21

$5\times 10^{-4}$ $2.59\times 10^{47}$ 0.777 280

**Table 1:** Characteristic values for the VLTP, for various MTS values. Note the dispersion in born again times according to the adopted MTS value. The third column shows characteristic time for the duration of the peak of proton burning. The born-again times correspond to the time interval from the moment of maximum $T_{\rm eff}$ after the H burning (and at high luminosity) until $\log{T_{\rm eff}}=3.8$ is reached for the first time.
MTS	$\int{L{\rm _H dt}}$ [erg]	$\Delta t$ [days]	Born-again
		$L_{\rm H}>(e^{-1} \times {L_{\rm H}}_{\rm max} )$	time-scale [yr]
$1\times 10^{-5}$	$4.5\times 10^{47}$	0.113	8.7
$3\times 10^{-5}$	$4.31\times 10^{47}$	0.133	10.3
$1\times 10^{-4}$	$3.75\times 10^{47}$	0.209	21
$5\times 10^{-4}$	$2.59\times 10^{47}$	0.777	280

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