Not exact matches
In the 1970s, astronomers Vera Rubin and Kent Ford used the same basic arguments to show, in
much more convincing detail, that spiral
galaxies appear to keep their
shapes because
of the gravitational glue from nearby dark matter.
A new computer re-enactment
of billions
of years
of galactic evolution suggests that the Milky Way owes
much of its current
shape to interactions with a nearby dwarf
galaxy.
From Earth, MCG -6-30-15 doesn'tlook like
much: It's a lenticular
galaxy, a lens -
shaped blob
of starswithout the photogenic spiral arms that typify our Milky Way
galaxy.