Stellar Velocity Dispersion of the Host Bulge in The Two Body Problem Formulas

Stellar Velocity Dispersion of the Host Bulge is the statistical dispersion of velocities about the mean velocity for a group of astronomical objects. And is denoted by σ. Stellar Velocity Dispersion of the Host Bulge is usually measured using the Kilometer per Second for Speed. Note that the value of Stellar Velocity Dispersion of the Host Bulge is always positive.

The Two Body Problem formulas that make use of Stellar Velocity Dispersion of the Host Bulge

fxRadius of Sphere of Influence( Black Hole)Go

FAQ

What is the Stellar Velocity Dispersion of the Host Bulge?

Stellar Velocity Dispersion of the Host Bulge is the statistical dispersion of velocities about the mean velocity for a group of astronomical objects. Stellar Velocity Dispersion of the Host Bulge is usually measured using the Kilometer per Second for Speed. Note that the value of Stellar Velocity Dispersion of the Host Bulge is always positive.

Can the Stellar Velocity Dispersion of the Host Bulge be negative?

No, the Stellar Velocity Dispersion of the Host Bulge, measured in Speed cannot be negative.

What unit is used to measure Stellar Velocity Dispersion of the Host Bulge?

Stellar Velocity Dispersion of the Host Bulge is usually measured using the Kilometer per Second[km/s] for Speed. Meter per Second[km/s], Meter per Minute[km/s], Meter per Hour[km/s] are the few other units in which Stellar Velocity Dispersion of the Host Bulge can be measured.

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