Abstract
Luminous Compact Blue Galaxies (LCBGs) are ∼L*, blue, high surface brightness, high metallicity, vigorously starbursting galaxies with an underlying older stellar population [1, 2]. They include a variety of morphological types, such as spiral, polar-ring, interacting/merging and peculiar galaxies. They have optical diameters of a few kpc, but are more luminous and more metal rich than the Blue Compact Dwarf Galaxies widely studied in the nearby Universe, e.g. [3, 4].
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Garland, C.A., Pisano, D.J., Williams, J.P., Guzmán, R., Castander, F.J. (1997). The Neutral ISM in Nearby Luminous Compact Blue Galaxies. In: Pfalzner, S., Kramer, C., Straubmeier, C., Heithausen, A. (eds) The Dense Interstellar Medium in Galaxies. Springer Proceedings in Physics, vol 91. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-18902-9_25
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DOI: https://doi.org/10.1007/978-3-642-18902-9_25
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