The Chemical Composition and Age of the Blue Compact Dwarf Galaxy Haro 2

Spectroscopic observations are presented of the central star-forming nebula in the Blue Compact Dwarf Galaxy Haro 2 (Mrk 33). Using the strengths of various emission lines, it is found that (1) the electron temperature is roughly 9250 K, and (2) the O abundance is comparable with that of the LMC. Weak Mg b λ 5175 and Fe I λ 5335 absorption lines have also been identified. An effort has been made to investigate the origin of these lines using synthetic spectra. It is concluded that, contrary to the findings of Loose and Thuan (1986), Haro 2 probably contains an old stellar substrate. Finally, it is suggested that Haro 2 may eventually evolve into a nucleated dwarf elliptical galaxy.