Along with these complex stellar characteristics are those of our Milky Way;
the whole central bulge rotates around the galactic centre.
Not exact matches
They found that the mass in the
central bulge (regardless of how big the disk surrounding it may be) is the key to knowing the colour of the
whole galaxy.
Team member Erica Nelson, of Yale University, added: «These galaxies show us the
whole Milky Way grew at the same time, unlike more massive elliptical galaxies, in which the
central bulge forms first.»