Proper-Motion Studies of Galactic Globular Clusters

Add to your list(s) Download to your calendar using vCal

• Laura Watkins (ESO)
• Thursday 28 February 2019, 16:00-17:00
• Sackler Lecture Theatre, IoA (tea at 3:30 pm).

If you have a question about this talk, please contact ma557.

Globular clusters (GCs) are old, collisional systems so the stars inside them interact on short timescales and have had a very long time in which to do so. These many and frequent interactions significantly affect both the structural and kinematic properties of GCs, so by studying their structure and kinematics we can learn about their evolution.

Some effects manifest as anisotropy in the velocity distributions, which require at least two (but preferably three) components of velocity information, and can only be seen with proper motion data. The Hubble Space Telescope and Gaia are highly complementary: HST has the depth to provide kinematics for a wide range of stellar masses, while Gaia has the spatial coverage to study changes across the whole cluster all the way out to its edges.

In my talk, I will focus on what we are learning about GCs from analysis of their kinematics using existing data, particularly proper motions from HST and Gaia. I will also discuss the advances that current and future telescopes will enable.

This talk is part of the Institute of Astronomy Colloquia series.

This talk is included in these lists:

• Combined External Astrophysics Talks DAMTP
• Cosmology lists
• Cosmology, Astrophysics and General Relativity
• Institute of Astronomy Colloquia
• Institute of Astronomy Talk Lists
• Kavli Institute for Cosmology Talk Lists
• Priscilla
• Sackler Lecture Theatre, IoA (tea at 3:30 pm)

Note that ex-directory lists are not shown.