Bright Stars and Recent Star Formation in the Irregular Magellanic Galaxy NGC 2366
The stellar content of the Im galaxy NGC 2366 is discussed on the basis of CCD BVR photometry. The three brightest blue and red stars have been used to estimate its distance, obtaining a value of 2.9 Mpc. The spatial distribution of the young stellar population is discussed in the light of the integrated color indices and the color-magnitude
Aparicio, A. et al.
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1995