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Comment on "Equation of state of dense and magnetized fermion system"
A. Y. Potekhin, D. G. Yakovlev
Contrary to what is claimed by Ferrer et al. [Phys. Rev. C 82, 065802 (2010)], the magnetic field of a neutron star cannot exceed 10^{19} G and the thermodynamic pressure of dense…
Chandra Phase-Resolved X-ray Spectroscopy of the Crab Pulsar II
Martin C. Weisskopf, Allyn F. Tennant, Dmitry G. Yakovlev +5
We present a new study of the X-ray spectral properties of the Crab Pulsar. The superb angular resolution of the Chandra X-ray Observatory enables distinguishing the pulsar from th…
Cooling neutron star in the Cassiopeia~A supernova remnant: Evidence for superfluidity in the core
Peter S. Shternin, Dmitry G. Yakovlev, Craig O. Heinke +2
According to recent results of Ho & Heinke (2009) and Heinke & Ho (2010), the Cassiopeia A supernova remnant contains a young neutron star which has carbon atmosphere and shows not…