about
Sharp knee phenomenon of primary cosmic ray energy spectrumThe influence of the enhanced vector meson sector on the properties of the matter of neutron stars.Forecasting neutron star temperatures: predictability and variability.A highly resistive layer within the crust of X-ray pulsars limits their spin periodsDensity-shear instability in electron magneto-hydrodynamicsHall effect in neutron star crusts: evolution, endpoint and dependence on initial conditions
P2860
description
2008 nî lūn-bûn
@nan
2008年の論文
@ja
2008年論文
@yue
2008年論文
@zh-hant
2008年論文
@zh-hk
2008年論文
@zh-mo
2008年論文
@zh-tw
2008年论文
@wuu
2008年论文
@zh
2008年论文
@zh-cn
name
Physics of Neutron Star Crusts.
@en
Physics of Neutron Star Crusts.
@nl
type
label
Physics of Neutron Star Crusts.
@en
Physics of Neutron Star Crusts.
@nl
prefLabel
Physics of Neutron Star Crusts.
@en
Physics of Neutron Star Crusts.
@nl
P2860
P356
P1476
Physics of Neutron Star Crusts
@en
P2093
Pawel Haensel
P2860
P2888
P356
10.12942/LRR-2008-10
P577
2008-12-12T00:00:00Z
P5875
P6179
1032486057