Changes between Version 6 and Version 7 of Talks/Falll2011/SpecialSeminars/111110a
- Timestamp:
- 11/08/11 13:36:10 (15 years ago)
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Talks/Falll2011/SpecialSeminars/111110a
v6 v7 19 19 ~0.5-2 MK thermal radiation from their magnetic polar caps. Realistic 20 20 modelling of this surface emission, including full relativistic and 21 atmospheric effect , has the potential to yield stringent constraints on21 atmospheric effects, has the potential to yield stringent constraints on 22 22 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
