Thermal emission from Isolated Neutron Stars and their surface magnetic   field: going quadrupolar?
  In the last few years considerable observational resources have been devoted to study the thermal emission from isolated neutron stars. Detailed XMM and Chandra observations revealed a number of features in the X-ray pulse profile, like asymmetry, energy dependence, and possible evolution of the pulse profile over a time scale of months or years. Here we show that these characteristics may be explained by a patchy surface temperature distribution, which is expected if the magnetic field has a complex structure in which higher order multipoles contribute together with the dipole. We reconsider these effects from a theoretical point of view, and discuss their implications to the observational properties of thermally emitting neutron stars. 
Silvia Zane (MSSL, UCL, UK), Roberto Turolla (Dept of Physics, Univ.   of Padova, Italy)