  Ring nebulae are often found around massive stars such as Wolf-Rayet stars,
OB and Of stars and Luminous Blue Variables (LBVs). In this paper we report on
two ring nebulae around blue supergiants in the Large Magellanic Cloud. The
star Sk-69 279 is classified as O9f and is surrounded by a closed shell with a
diameter of 4.5 pc. Our echelle observations show an expansion velocity of 14
km/s and a high [N II]6583A/H alpha ratio. This line ratio suggests nitrogen
abundance enhancement consistent with those seen in ejectas from LBVs. Thus the
ring nebula around Sk-69 279 is a circumstellar bubble. The star Sk-69 271, a
B2 supergiant, is surrounded by an H alpha arc resembling an half shell.
Echelle observations show a large expanding shell with the arc being part of
the approaching surface. The expansion velocity is about 24 km/s and the [N
II]6583A/H alpha is not much higher than that of the background emission. The
lack of nitrogen abundance anomaly suggests that the expanding shell is an
interstellar bubble with a dynamic age of 2 10^5 yr.
