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We discuss the determination of neutron star masses in X-ray binaries and explain the importance of such measurements. Examples are given of two of our recent neutron star mass determinations, in Cen X-3 and Vela X-1. We then discuss prospects for improving such measurements with SALT and the possibility of determining only the seventh neutron star mass in such a system by measuring the radial velocity curve of the recently discovered counterpart to the X-ray pulsar OAO1657--415.
|Item Type:||Conference Item|
|Academic Unit/Department:||Science > Physical Sciences
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Users 6042 not found.|
|Date Deposited:||07 Sep 2006|
|Last Modified:||29 Feb 2016 07:00|
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