Selection limits on galaxies
Plot (from Keel) of luminosity (MB and physical size (D25 in kpc) for the galaxies in RC2. Also shown are lines that would exclude objects from being recognized as galaxies: very compact galaxies would look like stars (upper line) while galaxies with surface brightness well below the sky would also go unrecognized (LSB galaxies: lower line).
We now know luminous compact galaxies are not common; low luminosity LSB galaxies are common (e.g. dwarf spheroidals); but high luminosity LSB galaxies are not very common, though some do exist (See below).
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Giant LSB galaxy: Malin 1
The prototype luminous (MB ~ -22) low surface brightness (LSB) galaxy" "Malin 1". Left: normal look-up. Right: highly stretched to see low surface brightness features (images from Bothun, taken from Keel). It is now thought that these galaxies are not a major population. In this case, there is a smaller "normal" disk in the center, and the very large extended disk is similar to extended HI disks in other spirals -- except this one has associated star formation.
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