Correction of the orbital mass of double galaxies estimation
L. Belyaeva, S. Parnovsky
TL;DR
This paper presents a refined statistical method for estimating the mass of double galaxies in circular orbits, providing confidence intervals for various confidence levels.
Contribution
It introduces an improved estimation technique that enhances accuracy and reliability in determining galaxy masses from orbital data.
Findings
More precise mass estimates for double galaxies
Confidence intervals for different confidence levels
Enhanced statistical methodology
Abstract
We obtain a more accurate statistical estimation of the mass of double galaxies moving in circular orbits, including confidence intervals for different confidence levels.
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Scientific Research and Discoveries · Astronomy and Astrophysical Research