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
Hauptverfasser: Campbell, David J. R., Frenk, Carlos S., Jenkins, Adrian, Eke, Vincent R., Navarro, Julio F., Sawala, Till, Schaller, Matthieu, Fattahi, Azadeh, Oman, Kyle A., Theuns, Tom
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Sprache:eng
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