This work presents UBV photometry of the stellar populations associated with seven superbubble nebulae and five classical H II regions in the Large Magellanic Cloud. Although the nebular morphology of the superbubbles appears to be substantially evolved compared to the classical nebulae, the color-magnitude diagrams do not reveal any noticeable correlation between the resident stellar population and nebular morphology. The photometry presented here will be used in a forthcoming paper to examine further the stellar content and dynamics of these superbubbles.
Cone search capability for table J/ApJS/104/71/table4a (Photometry for DEM 25)
Cone search capability for table J/ApJS/104/71/table4b (Photometry for DEM 31)
Cone search capability for table J/ApJS/104/71/table4c (Photometry for DEM 50)
Cone search capability for table J/ApJS/104/71/table4d (Photometry for DEM 106)
Cone search capability for table J/ApJS/104/71/table4e (Photometry for DEM 192)
Cone search capability for table J/ApJS/104/71/table4i (Photometry for DEM 10b)
Cone search capability for table J/ApJS/104/71/table4j (Photometry for DEM 66)
Cone search capability for table J/ApJS/104/71/table4k (Photometry for DEM 197)
Cone search capability for table J/ApJS/104/71/table4f (Photometry for DEM 226)
Cone search capability for table J/ApJS/104/71/table4g (Photometry for DEM 231)
Cone search capability for table J/ApJS/104/71/table4h (Photometry for DEM 301)
Cone search capability for table J/ApJS/104/71/table4l (Photometry for DEM 243)
Cone search capability for table J/ApJS/104/71/table4m (Photometry for DEM 293)