Showing 801 - 820 results of 1,510 for search '"neutron stars"', query time: 1.34s Refine Results
  1. 801
    ... the Sun, the Earth, or neutron stars. There, they can become non-extremal either from merging...
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    Article
  2. 802
    by Roberto Taverna, Roberto Turolla
    Published 2018-03-01
    ... neutron stars endowed with an ultra-strong magnetic field ( B ≈ 10 14 – 10 15 G...
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    Article
  3. 803
    by Ye-Fei Yuan, Xin-Yue Shi
    Published 2019-08-01
    ... might potentially happen in the atmosphere of white dwarfs, neutron stars or even that of stellar...
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    Article
  4. 804
  5. 805
    ... binaries or, in one case, from coalescing neutron stars. These observations opened up the era...
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    Article
  6. 806
    by Masaomi Tanaka
    Published 2016-01-01
    ... of two neutron stars or a neutron star and a black hole). Kilonova/macronova is emission powered...
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    Article
  7. 807
  8. 808
    by Pallanca, Cristina <1985>
    Published 2014
    ...Millisecond Pulsars (MSPs) are fast rotating, highly magnetized neutron stars. According...
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    Doctoral Thesis
  9. 809
    by Barnes, A.
    Published 2004
    ..., the standard shocktube problem is used to test the code, and perturbed, rotating neutron stars are studied....
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  10. 810
    by Contenta, Filippo
    Published 2017
    ... the final star cluster properties, such as the neutron stars natal kick distribution. I conclude, through a...
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  11. 811
    by Carlos Herdeiro, Eugen Radu, D. H. Tchrakian
    Published 2021-04-01
    ... squared Gauss–Bonnet (GB) term, compact objects such as neutron stars and black holes (BHs) can...
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    Article
  12. 812
    by Massart, V., Paranjape, M.B
    Published 2022
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    Article
  13. 813
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  14. 814
  15. 815
    by Arnab Sarkar, Amna Ali, Salah Nasri
    Published 2021-08-01
    ... sufficiently accelerated motion of charged stars (specially neutron stars) or charged stellar mass black holes...
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    Article
  16. 816
    ... are generalizations of the light cylinders found around magnetized neutron stars. In both cases, we give the explicit...
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    Article
  17. 817
    by S. B. Popov, M. E. Prokhorov, V. M. Lipunov
    Published 2017-03-01
    ... with neutron stars and with black holes) for different parameters of the IMF - slopes: α = 1, α = 1.35 and α...
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    Article
  18. 818
    ... birefringence of GWs. If a nearly edge-on binary neutron-stars with observed electromagnetic counterparts at 40...
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    Article
  19. 819
    by Bell, Elizabeth
    Published 2005
    ..., then the equilibrium ratio of protons to neutrons inside high density neutron stars can be inferred, allowing...
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  20. 820
    by Charbonneau, Arthur James
    Published 2011
    ... fields, dense matter, and parity violation. We propose that such a current exists in the cores of neutron...
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