Application of the virial theorem to clusters of galaxies with unseen mass
Jr. Smith H.
Abstract
Jr. Smith H.
Abstract
Application of the virial theorem to N-body systems with various distributions of unseen mass and a reasonable set of initial conditions gives mass values that are overestimates, both for cylindrical samples and for the entire system. The overestimation in the latter case is as much as a factor 3.5-4 and is implicit in earlier work by Limber.
OpenAlex reports 15 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
Application of the virial theorem to N-body systems with various distributions of unseen mass and a reasonable set of initial conditions gives mass values that are overestimates, both for cylindrical samples and for the entire system. The overestimation in the latter case is as much as a factor 3.5-4 and is implicit in earlier work by Limber.
Key concepts: Virial theorem, Virial mass, Physics, Galaxy, Astrophysics, Galaxy cluster, Theoretical physics