Unlike previous SDSS surveys, they are not only mapping the centers of galaxies where supermassive black holes live, but
the outer edges of the galaxies as well, which allowed them to discover the red geyser galaxy.
They did this by measuring the acceleration of clouds orbiting on
the outer edges of a galaxy, which enabled them to calculate the mass required to cause that acceleration.
Not exact matches
These
galaxies brushed past each other — scraping the
edges of their
outer spiral arms — in what is likely the first encounter
of an eventual merger.
This small
galaxy has now been almost completely destroyed, but signs
of the collision persist in the backward motion
of gas at the
outer edge of M64.