Abstract:
The Large Magellanic Cloud has been surveyed on ultralow dispersion (10,000 A/mm) plates taken with the 102-centimeter reflector at Kavalur. Many new red and blue stars were found. The LMC bar was found to have a strong component of red stars and a very weak component of faint OB stars. In general the regions other than the bar contain very luminous OB stars, faint OB stars and a few very red stars. The 30 Doradus complex is rich in luminous red and blue stars