If the source is moving away from the observer, the spectral line will be shifted to a longer wavelength.
The 21-cm Line
Slide 12
The relative change in wavelength is related to the source’s velocity.
Stationary
Moving slow
Moving fast
The 21-cm Line
Slide 13
Uses of the 21-cm line
The Milky Way has over 3 billion solar masses of hydrogen gas.
Enough hydrogen atoms so that the 21-cm line is easily detected by radio telescopes.
Therefore, it is the best way to map the structure of the galaxy.
The 21-cm Line
Slide 14
Example: Rotation of the Milky Way
The 21-cm Line
Image from Richard Powell www.atlasoftheuniverse.com