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   PR # 42048
   We propose to complete our project to observe bright globular cluster
   LMXBs with an ASCA AO-4 observation of X0513-401 (NGC 1851).
   X0513-401 is the final source in the program; although C time was
   awarded in ASCA AO-3, it was not included in the final timeline. The
   project aims to relate the abundances in the sources with those of
   the surrounding clusters, study the continuum and burst emission, and
   search for lines and edges; for X0513-401 we will also search for
   low-level orbital modulations. X0513-401 is important for this study
   as it is located in a metal-poor cluster. In addition, we have
   obtained XTE AO-1 time which can be scheduled simultaneously,
   enabling us to correlate the fast timing activity of the source with
   its spectral state.
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