Figure 3.
Cumulative root-mean-square (rms) velocity dispersion profiles. The plot shows the rotation-included velocity dispersion profiles within a certain radius for all (top panel), blue (central panel) and red GCs (bottom panel). A running mean is used. Different colours represent different galaxies. Most of the profiles are generally flat at all radii.

Cumulative root-mean-square (rms) velocity dispersion profiles. The plot shows the rotation-included velocity dispersion profiles within a certain radius for all (top panel), blue (central panel) and red GCs (bottom panel). A running mean is used. Different colours represent different galaxies. Most of the profiles are generally flat at all radii.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close