The Galactic Bulge Survey
The images linked below show some of the tools that we use
to identify optical stars related to an X-ray source. First, we use
the accurate astrometry
provided by the Chandra satellite. Next we make use of
the three color information provide
by our optical data to select those sources which have an H_alpha
excees. Note, however, that not all sources of interest have such an
excess since some sources are H-poor (e.g. ultra-compact X-ray
binaries). Finally, we obtain
classification spectra of all optical counterparts to the X-ray
sources. In the case linked above the source is a Cataclysmic Variable
showing a strong H_alpha emission peak.
|