A Star-Bursting Galaxy Born from the Collision of Dwarfs

What happens when the large-scale drama of a violent galaxy merger plays out on small scales for a pair of dwarf galaxies? New observations document the scene of a recent dwarf-galaxy collision.Dramatic EncountersThe Antennae Galaxies are an example of a starburst galaxy with rapid star-formation activity driven by a recent merger. [NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration]When two galaxies merge, the collision can have dramatic consequences particularly if the galaxies are rich in gas. The gravitational interaction of galaxies oscillating during a merger drives shock waves through their gas. This can trigger bursts of star formation, launch jets from active galactic nuclei, and result in the eventual formation of a new galaxy with drastically different morphology than the original merging pair.Weve seen this drama play out on large scales between giant galaxies, but we know a lot less about what happens when dwarf galaxies collide. Dwarf galaxies are the most abundant type of galaxy in the universe, but theyre also very small and faint. This poses a significant challenge to finding and studying dwarfs which means theres a lot we dont know about how the mergers of dwarf galaxies impact overall star formation and the shape of the new galaxy that forms in the collision.This g-band image of VCC 848 better shows the galaxys three extended shell-like structures (outlined with red arcs) surrounding the central body of stars. [Adapted from Zhang et al. 2020]Fortunately, we may now have an opportunity to learn more. In a recent publication led by Hong-Xin Zhang (University of Science and Technology of China), a team of scientists reports on the discovery of a small, compact galaxy formed by the collision of two dwarfs.Feeling Shell-ShockedVCC 848 is whats known as a blue compact dwarf galaxy a small galaxy thats actively undergoing a burst of star formation. Located in the outskirts of the Virgo Cluster some 65 million light-years away, this little dwarf shows telltale signs of a recent merger: careful analysis reveals a complex set of three extended shell-like structures of stars around the bright stellar main body.Shell structures which, previously, had only been detected in larger galaxies are known to be a signature of a recent minor or major galaxy merger; they are formed as the merger sends ripples through the galaxy and disrupts its structure. The detection of these shells in such a small galaxy provides evidence that were looking at the recent merger of two dwarfs.A Flurry of ActivityZhang and collaborators use their observations of VCC 848 made with the MegaCam instrument on the CanadaFranceHawaii Telescope in Hawaii to analyze the stars of the galaxy and learn more about its history.The average formation rate per billion years of star clusters above a certain birth mass, for the age intervals of 01 Gyr and 113 Gyr. This indicates that star formation was significantly more active in the last billion years. [Adapted from Zhang et al. 2020]They determine that the two dwarfs that collided were likely similar in mass to within a factor of a few, and the merger triggered a burst of star formation over the past billion years that was ~710 times higher than normal. This enhancement in star formation peaked near the center of the galaxy a few hundred million years ago, and its since declined; current star formation activity is primarily in VCC 848s outer regions.VCC 848 is just one of several blue compact dwarfs with hints of tidal shells that the authors uncovered in their survey, so theres more data on the way! We have a lot more to learn about what happens when tiny galaxies collide.CitationThe Blue Compact Dwarf Galaxy VCC 848 Formed by DwarfDwarf Merging, Hong-Xin Zhang et al 2020 ApJL 891 L23. doi:10.3847/2041-8213/ab7825