How Well Can SIM Lite Measure the Parameters of Neutron Star and Black Hole Binaries?

Astronomy and Astrophysics – Astronomy

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With microarcsecond astrometry, we know that the sky will come alive for the Space Interferometry Mission as it uncovers stellar motions that have previously been hidden from view. In addition to SIM's ability to provide parallax and proper motion measurements for any star in our Galaxy brighter than a V-magnitude of 20, SIM will also have the capability to study orbital motions for many different types of systems, including X-ray binaries. This presentation focuses on the advances that SIM Lite will allow in the study of neutron star and black holes. In particular, we will discuss our program to simulate SIM Lite observations to determine how accurately this mission will be able to measure the masses of compact objects in X-ray binaries. Such measurements are important for placing constraints on the neutron star equation of state as well as improving our understanding of stellar evolution and compact object formation.

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