First detection of a magnetic field in low-luminosity B[e] stars - New scenarios for the nature and evolutionary stages of FS CMa stars

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Table 2

GALEX data.

	Brightness	Intrinsic	Flux
		brightness
	(mag)	(mag)	(μJ)
FUV	12.527 ± 0.004	11.847	35 400 ± 112
NUV	12.485 ± 0.002	11.720	36 800 ± 67

Notes. The intrinsic brightness is calculated for the value of E(B − V) tabulated in the GALEX catalog (~0.083) and errors are commented in the text. The FUV camera wavelength region is from 1344 to 1786 Å, and NUV region from 1771 to 2831 Å.

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