Determining the Physical Masses of Exoplanets Observed by Radial Velocity Measurements: A Review of Methods and Solutions, Results, and New Questions from Published Data
摘要
Abstract—
A review of scientific publications devoted to the mathematical problem of transition from distributions of minimum masses of exoplanets discovered by the radial velocity method to their distribution by physical masses is presented. The methods for solving this problem, both analytical and numerical, are described, and the results obtained are discussed. In conclusion, some unresolved issues requiring further discussion are described.