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zadetkov: 13.230
1.
  • The Radius of PSR J0740+662... The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
    Miller, M. C.; Lamb, F. K.; Dittmann, A. J. ... Astrophysical journal. Letters, 09/2021, Letnik: 918, Številka: 2
    Journal Article
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    Abstract PSR J0740+6620 has a gravitational mass of 2.08 ± 0.07 M ⊙ , which is the highest reliably determined mass of any neutron star. As a result, a measurement of its radius will provide unique ...
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2.
  • PSR J0030+0451 Mass and Rad... PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
    Miller, M. C.; Lamb, F. K.; Dittmann, A. J. ... Astrophysical journal. Letters, 12/2019, Letnik: 887, Številka: 1
    Journal Article
    Recenzirano
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    Neutron stars are not only of astrophysical interest, but are also of great interest to nuclear physicists because their attributes can be used to determine the properties of the dense matter in ...
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3.
  • Constraints on the Dense Ma... Constraints on the Dense Matter Equation of State and Neutron Star Properties from NICER’s Mass–Radius Estimate of PSR J0740+6620 and Multimessenger Observations
    Raaijmakers, G.; Greif, S. K.; Hebeler, K. ... Astrophysical journal. Letters, 09/2021, Letnik: 918, Številka: 2
    Journal Article
    Recenzirano
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    Abstract In recent years our understanding of the dense matter equation of state (EOS) of neutron stars has significantly improved by analyzing multimessenger data from radio/X-ray pulsars, ...
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4.
  • A NICER View of PSR J0030+0... A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
    Riley, T. E.; Watts, A. L.; Bogdanov, S. ... Astrophysical journal. Letters, 12/2019, Letnik: 887, Številka: 1
    Journal Article
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    We report on Bayesian parameter estimation of the mass and equatorial radius of the millisecond pulsar PSR J0030+0451, conditional on pulse-profile modeling of Neutron Star Interior Composition ...
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5.
  • A NICER View of PSR J0030+0... A NICER View of PSR J0030+0451: Implications for the Dense Matter Equation of State
    Raaijmakers, G.; Riley, T. E.; Watts, A. L. ... Astrophysical journal. Letters, 12/2019, Letnik: 887, Številka: 1
    Journal Article
    Recenzirano
    Odprti dostop

    Both the mass and radius of the millisecond pulsar PSR J0030+0451 have been inferred via pulse-profile modeling of X-ray data obtained by NASA's Neutron Star Interior Composition Explorer (NICER) ...
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6.
  • Evolution of a buried magne... Evolution of a buried magnetic field in the central compact object neutron stars
    Ho, Wynn C. G. Monthly Notices of the Royal Astronomical Society, July 2011, Letnik: 414, Številka: 3
    Journal Article
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    The central compact objects are a newly emerging class of young neutron stars near the centre of supernova remnants. From X-ray timing and spectral measurements, their magnetic fields are determined ...
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7.
  • Using gravitational-wave da... Using gravitational-wave data to constrain dynamical tides in neutron star binaries
    Andersson, Nils; Ho, Wynn C. G. Physical review. D, 01/2018, Letnik: 97, Številka: 2
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    We discuss the role of dynamical tidal effects for inspiraling neutron star binaries, focusing on features that may be considered “unmodeled” in gravitational-wave searches. In order to cover the ...
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8.
  • Constraining the mass and r... Constraining the mass and radius of neutron stars in globular clusters
    Steiner, A W; Heinke, C O; Bogdanov, S ... Monthly Notices of the Royal Astronomical Society, 05/2018, Letnik: 476, Številka: 1
    Journal Article
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    Abstract We analyse observations of eight quiescent low-mass X-ray binaries in globular clusters and combine them to determine the neutron star mass–radius curve and the equation of state of dense ...
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9.
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10.
  • Direct Observation of the C... Direct Observation of the Cooling of the Cassiopeia A Neutron Star
    Heinke, Craig O; Ho, Wynn C. G Astrophysical journal. Letters, 08/2010, Letnik: 719, Številka: 2
    Journal Article
    Recenzirano

    The cooling rate of young neutron stars (NSs) gives direct insight into their internal makeup. Although the temperatures of several young NSs have been measured, until now a young NS has never been ...
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zadetkov: 13.230

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