Origin and Evolution of Neutron Star Magnetic Fields - if
... Neutron stars with young, high-mass companions (“high-mass X-ray binaries” or HMXBs) tend to appear as X-ray pulsars, in which the accreted material is presumably channelled by the magnetic field onto the polar caps. In some cases, cyclotron features have been found in the X-ray spectrum, correspondi ...
... Neutron stars with young, high-mass companions (“high-mass X-ray binaries” or HMXBs) tend to appear as X-ray pulsars, in which the accreted material is presumably channelled by the magnetic field onto the polar caps. In some cases, cyclotron features have been found in the X-ray spectrum, correspondi ...
Document
... on the same torus will move onto two different tori. • However, if potential is changed very slowly compared to all characteristic times associated with the motion on each torus, all phase points that are initially on a given torus will be equally affected by the variation in Potential • Any two sta ...
... on the same torus will move onto two different tori. • However, if potential is changed very slowly compared to all characteristic times associated with the motion on each torus, all phase points that are initially on a given torus will be equally affected by the variation in Potential • Any two sta ...
The role of black holes in galaxy formation and evolution
... In the first type of clusters, the gas has a high central density and radiates its thermal energy on a timescale tcool~ 3/2 kT / n2Λ that is usually less than a gigayear over much of the cluster cores. These clusters are called “cool core” clusters because T decreases toward the centre. However, “c ...
... In the first type of clusters, the gas has a high central density and radiates its thermal energy on a timescale tcool~ 3/2 kT / n2Λ that is usually less than a gigayear over much of the cluster cores. These clusters are called “cool core” clusters because T decreases toward the centre. However, “c ...
Physics 2010 Summer 2011 REVIEW FOR FINAL EXAM
... Driving along a country road you stop at a stop sign. There is another stop sign 1 km down the road. The speed limit is 40 mph. Your car’s maximum acceleration is 3 m/s2 and the maximum deceleration is 4 m/s 2. (a) (b) ...
... Driving along a country road you stop at a stop sign. There is another stop sign 1 km down the road. The speed limit is 40 mph. Your car’s maximum acceleration is 3 m/s2 and the maximum deceleration is 4 m/s 2. (a) (b) ...
Paper
... line defects such as vortices have cores where the density of condensed particles is necessarily zero to keep the order parameter single valued [11–13]. However, in condensates with an internal, spin degree of freedom, coreless vortices exist as spin textures [4,14]. Such structures are referred to ...
... line defects such as vortices have cores where the density of condensed particles is necessarily zero to keep the order parameter single valued [11–13]. However, in condensates with an internal, spin degree of freedom, coreless vortices exist as spin textures [4,14]. Such structures are referred to ...
