have a disk but no arms
have little or no excess gas and dust
Slide 62
any galaxy that isn’t a Spiral, Elliptical, or Lenticular
usually have lots of gas and dust and young stars
may have a distorted shape from interaction with another galaxy
Slide 63
Irregular Galaxies
Slide 64
We now think that galaxies in groups and clusters often collide
The Milky Way is moving at 300,000 mph toward the Andromeda Galaxy
They may collide in about 5 billion years
Stars don’t usually collide
New orbits, gas piles up to form new stars
Slide 65
Interacting
Slide 66
the Antennae or Mice
Slide 67
The occasional results of two galaxies colliding: ringed galaxies
Slide 68
Various galaxies (can you identify types?)
Slide 69
almost every medium to large galaxy we’ve check has a supermassive black hole at the center
the larger the galaxy, the more massive the black hole
we don’t know which comes first, the galaxy or the black hole
we think that these black holes are responsible for some of the galaxies with jets and lobes which give off radio waves, x-rays, etc.
Slide 70
Active galaxy
Slide 71
at the center of a large galaxy
Slide 72
the Local Group
includes the Milky Way, the Andromeda, and over 30 other smaller galaxies
the Virgo Cluster
hundreds to thousands of galaxies, 60 million light-years away
giant elliptical at center, formed by galactic cannibalism
the Local Group is “falling” toward the Virgo Cluster at 60 to 250 miles per second!
Slide 73
Coma Cluster
Slide 74
clusters are bound together in larger structures, called superclusters