MUSE observations of the blue compact dwarf galaxy Haro 14. Data analysis and first results on morphology and stellar populations

@article{Cairos2021MUSEOO,
  title={MUSE observations of the blue compact dwarf galaxy Haro 14. Data analysis and first results on morphology and stellar populations},
  author={Luz Marina Cair'os and J. N. Gonz'alez-P'erez and Peter M. Weilbacher and Russia Max-Planck-Institut fuer Astrophysik and Georg-August-Universitat and Gottingen and H Germany and Hamburger Sternwarte and Hamburg and Leibniz-Institut fur Astrophysik and Potsdam and Max Planck Institute for Solar System Research},
  journal={Astronomy \& Astrophysics},
  year={2021}
}
Investigations of blue compact galaxies (BCGs) are essential to advancing our understanding of galaxy formation and evolution. BCGs are low-luminosity, low-metallicity, gas-rich objects that form stars at extremely high rates, meaning they are good analogs to the high-redshift star-forming galaxy population. Being low-mass starburst systems, they also constitute excellent laboratories in which to investigate the star formation process and the interplay between massive stars and their… 

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MUSE observations of the blue compact dwarf galaxy Haro 14