Searching for exoplanets by detecting the motion of their stars

Part of the Springer Praxis Books book series (PRAXIS)


In the previous chapter 1 concentrated on those indirect methods where we infer the presence of a planet from its influence on the quantity of radiation we receive from this star or from some background star.


Radial Velocity Absorption Line Circular Orbit Angular Size Semimajor Axis 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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© Praxis Publishing Ltd. 2008

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