103 citations · 785 across the 27 of their papers we have counts for
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Three-dimensional magneto-thermal evolution of off-centred dipole magnetic field configurations in neutron stars
Andrei P. Igoshev, Rainer Hollerbach, Toby Wood
Off-centred dipole configurations have been suggested to explain different phenomena in neutron stars, such as natal kicks, irregularities in polarisation of radio pulsars and prop…
Three-Dimensional Magnetothermal Simulations of Magnetar Outbursts
Davide De Grandis, Roberto Turolla, Roberto Taverna +3
The defining trait of magnetars, the most strongly magnetized neutron stars (NSs), is their transient activity in the X/-bands. In particular, many of them undergo phases of enh…
X-ray Emission from Isolated Neutron Stars revisited: 3D magnetothermal simulations
Davide De Grandis, Roberto Taverna, Roberto Turolla +4
X-ray emission from the surface of isolated neutron stars (NSs) has been now observed in a variety of sources. The ubiquitous presence of pulsations clearly indicates that thermal…
3D Magneto-thermal Simulations of Tangled Crustal Magnetic Field in Central Compact Objects
Andrei P. Igoshev, Konstantinos N. Gourgouliatos, Rainer Hollerbach +1
Central compact objects are young neutron stars emitting thermal X-rays with bolometric luminosities in the range - erg/s. Gourgouliatos, Hollerbach and Igo…
Sleeping beasts: strong toroidal magnetic field in quiescent magnetars explains their large pulsed fraction
Andrei P. Igoshev, Rainer Hollerbach, Toby Wood +1
Magnetars are neutron stars (NSs) with extreme magnetic fields of strength - G. They exhibit transient, highly energetic events, such as short X-ray fl…
3D modelling of magneto-thermal evolution of neutron stars: method and test cases
Davide De Grandis, Roberto Turolla, Toby S. Wood +3
Neutron stars harbour extremely strong magnetic fields within their solid outer crust. The topology of this field strongly influences the surface temperature distribution, and henc…