A peculiar galaxy is a galaxy of unusual size, shape, or composition.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> Between five and ten percent of known galaxies are categorized as peculiar.<ref name=":1">Template:Cite book</ref> Astronomers have identified two types of peculiar galaxies: interacting galaxies and active galactic nuclei (AGN).<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>
When two galaxies come close to each other, their mutual gravitational forces can cause them to acquire highly irregular shapes.<ref name=":0">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> The terms 'peculiar galaxy' and 'interacting galaxy' have now become synonymous because the majority of peculiar galaxies attribute their forms to such gravitational forces.<ref name=":1" />
FormationEdit
Scientists hypothesize that many peculiar galaxies are formed by the collision of two or more galaxies.<ref name=":0" /> As such, peculiar galaxies tend to host more active galactic nuclei than normal galaxies, indicating that they contain supermassive black holes.<ref name=":1" /><ref name=":0" /> Many peculiar galaxies experience starbursts, or episodes of rapid star formation, due to the galaxies merging.<ref name=":1" /> The periods of elevated star formation and the luminosity resulting from active galactic nuclei cause peculiar galaxies to be slightly bluer in color than other galaxies.<ref name=":1" />
Studying peculiar galaxies can offer insights on other types of galaxies by providing useful information on galactic formation and evolution.<ref name=":1" /> Arp mapped peculiar galaxies in his 1966 Atlas of Peculiar Galaxies. Arp states that "the peculiarities of the galaxies pictured in this Atlas represent perturbations, deformations, and interactions which should enable us to analyze the nature of the real galaxies which we observe and which are too remote to experiment on directly."
NotationEdit
Peculiar galaxies are notated by an additional "p" or "pec" (depending on the exact convention) after the Hubble type of the galaxy.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>