| This section will introduce how our 
							Milky Way galaxy 
							evolved. The subject of
							galaxies themselves have 
							been left to the
							Cosmology section. However, before astronomers 
							can understand how other 
							galaxies evolve, we must 
							study our own 
							galaxy.
 Theories of the evolution of 
							our galaxy - and any other  - is under 
							continual refinement. Much of what we understand 
							about galactic formation is based on what we know 
							about
							Dark Matter. In a way, galactic formation is similar to 
							stellar formation, only on a much larger scale. With 
							the early Universe mixed with 
							Dark Matter and gases 
							containing molecular hydrogen, collisions eventually 
							occurred. Collisions led to conservation of energy 
							eventually resulting in collapse. There are two 
							methods of collapse: 
								
								Stars form early out of fragmentation, 
								resulting in shrinking and forming of elliptical 
								galaxies and
								globular clustersCloud shrinks faster resulting in rotation 
								of the cloud, then 
								star formation occurs So for elliptical 
								galaxies,
								stars formed 
								first. Spiral 
								galaxies like our 
								Milky Way formed 
								their
								stars later - after the cloud began 
								rotation. But what about the spiral structure? The leading theory is that the spiral 
								structure of our 
								galaxy is a consequence of the 
								distribution of
								OB Associations and hot
								stars. 
								In addition, Density Waves are believed to 
								travel through the disk stimulating 
								star birth 
								in their wake. Standard rotation does not explain the spiral 
								structure since the end result is what is called 
								the "winding problem." 
								 (Image credit: Brooks/Cole Thomson Learning)
 The spiral arms will overtake each other. 
								Here is an image that gives an example of the 
								density wave-OB Association (and hot
								star) 
								theory of spiral structure. 
								 This is a composite ultraviolet and infrared 
								image of M81. The infrared (shown in red) shows 
								the distribution of "normal" 
								stars. The blue 
								indicates the hot 
								OB type
								stars. Compare the above image with the true color 
								image below: 
								 It is clear that the hot 
								OB type
								stars are 
								tracing the spiral structure of the 
								galaxy. If 
								we could have a top-down view of our own 
							galaxy, 
								there is no doubt the view would be the same. 
								Much of what we learn about galactic formation 
								and evolution come from 
								computer simulations. 
								The study of
								Dark Matter
								and galactic formation 
								as well as the evolution of our 
								Universe all go 
								hand-in-hand - so stay tuned! Back 
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