On Rotation Curve Analysis
Kevin Kadowaki
TL;DR
This paper critically examines existing analytical methods for calculating galactic masses from rotation curves, highlighting flaws in previous approaches to improve future analysis accuracy.
Contribution
It identifies flaws in current methods for analyzing rotation curves and suggests the need for revised analytical techniques.
Findings
Current methods are flawed in their analysis of rotation curves
Revised techniques are necessary for accurate galactic mass estimation
The paper provides insights into improving rotation curve analysis
Abstract
An analysis of analytical methods used for computing galactic masses on the basis of rotation curves (Saari 2015) is shown to be flawed.
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Taxonomy
TopicsInertial Sensor and Navigation · Robotic Mechanisms and Dynamics