Eclipsing Binaries in Globular Clusters


My dissertation research with Prof. Mario Mateo involves a monitoring survey of 10 Galactic globular star clusters with the aim of finding eclipsing binary stars around the main-sequence turnoff. The simultaneous photometric and spectroscopic analysis of these systems can be used to to directly determine the distances to these systems and to calculate turnoff masses for cluster stars, thus providing a fundamental check of stellar models at low metallicity.

An interesting side project in the search for binary stars has been the creation of differential extinction maps for the target globular clusters. That is, we determined how much extinction light from different parts of the cluster suffers due to dust along the line of sight to the respective cluster.

You may see the following:

 

Click to see a color image of the globular clusters M10, M12, M92, NGC 5053, or NGC 3201. All are color composite images taken with either the MDM 1.3m telescope or the Las Campanas 1m telescope.