Changes between Version 7 and Version 8 of Talks/Falll2011/SpecialSeminars/111110a
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Talks/Falll2011/SpecialSeminars/111110a
v7 v8 20 20 modelling of this surface emission, including full relativistic and 21 21 atmospheric effects, has the potential to yield stringent constraints on 22 the elusive neutron star equation of state. In this talk I will22 the elusive neutron star equation of state. In this talk, I will 23 23 summarize the current state of affairs and future prospects in the study 24 24 of millisecond pulsars at X-ray energies.
