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A Near Infrared Study of Blue Dwarf Galaxies
Publications of the Astronomical Society of the Pacific, 1997Blue Dwarf Galaxies (BDG) are objects of low luminosity (MVge-18) and very blue visible colors. Both the colors and the presence of narrow emission lines in their spectra are usually interpreted to result from intense episodes of star formation. The metallicity of the BDG is usually low with values in the range 10-2-1~Zodot.
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