Cooling neutron star in the Cassiopeia A supernova remnant: evidence for superfluidity in the core
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QCD and strongly coupled gauge theories: challenges and perspectives.Revealing the physics of R modes in low-mass x-ray binaries.Lieb-Liniger-like model of quantum solvation in CO-(4)HeN clusters.Magnetic fields in superconducting neutron stars.Pulsar glitches: the crust is not enough.Imprints of superfluidity on magnetoelastic quasiperiodic oscillations of soft gamma-ray repeaters.A highly resistive layer within the crust of X-ray pulsars limits their spin periodsTests of the nuclear equation of state and superfluid and superconducting gaps using the Cassiopeia A neutron starHottest Superfluid and Superconductor in the Universe: Lessons from the Cooling of the Cassiopeia A Neutron StarThe neutron star in Cassiopeia A: equation of state, superfluidity, and Joule heating
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P2860
Cooling neutron star in the Cassiopeia A supernova remnant: evidence for superfluidity in the core
description
article
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в лютому 2011
@uk
name
Cooling neutron star in the Ca ...... for superfluidity in the core
@en
Cooling neutron star in the Ca ...... for superfluidity in the core
@nl
type
label
Cooling neutron star in the Ca ...... for superfluidity in the core
@en
Cooling neutron star in the Ca ...... for superfluidity in the core
@nl
prefLabel
Cooling neutron star in the Ca ...... for superfluidity in the core
@en
Cooling neutron star in the Ca ...... for superfluidity in the core
@nl
P2093
P2860
P1476
Cooling neutron star in the Ca ...... for superfluidity in the core
@en
P2093
Craig O. Heinke
Daniel J. Patnaude
Dmitry G. Yakovlev
Peter S. Shternin
Wynn C. G. Ho
P2860
P304
P356
10.1111/J.1745-3933.2011.01015.X
P577
2011-02-07T00:00:00Z
P818
P819
2011MNRAS.412L.108S