Table 3: X-ray luminosities (corrected for interstellar absorption) of V390 Aurigae in the 0.3-2 keV and 2-10 keV bands. The percentage contribution in luminosity of hot plasmas (kT>1 keV) is indicated between brackets.
Obs. $L_{\rm0.3-2~keV}$ $L_{\rm 2-10~keV}$ hr

(10³⁰ erg s^-1) (10³⁰ erg s^-1)

Rev. 135 3.90 0.30 - 0.86

(41%) (79%)

Rev. 232 5.27 0.61 - 0.79

(55%) (90%)

**Table 3:** X-ray luminosities (corrected for interstellar absorption) of V390 Aurigae in the 0.3-2 keV and 2-10 keV bands. The percentage contribution in luminosity of hot plasmas (kT>1 keV) is indicated between brackets.
Obs.	$L_{\rm0.3-2~keV}$	$L_{\rm 2-10~keV}$	hr
	(10³⁰ erg s^-1)	(10³⁰ erg s^-1)
Rev. 135	3.90	0.30	- 0.86
	(41%)	(79%)
Rev. 232	5.27	0.61	- 0.79
	(55%)	(90%)

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