Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses
Abstract The observed stellar kinematics of dispersion-supported galaxies are often used to measure dynamical masses. Recently, several analytical relationships between the stellar line-of-sight velocity dispersion, the projected (2D) or deprojected (3D) half-light radius and the total mass enclosed...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2017-08, Vol.469 (2), p.2335-2360 |
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Hauptverfasser: | , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
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