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相关论文: Constraints on Neutron Star Properties from X-ray …

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Abridged) We model the X-ray properties of millisecond pulsars (MSPs) by considering hot spot emission from a weakly magnetized rotating neutron star (NS) covered by an optically-thick hydrogen atmosphere. We investigate the limitations of…

天体物理学 · 物理学 2009-11-13 Slavko Bogdanov , Jonathan E. Grindlay , George B. Rybicki

I present an analysis of the deepest X-ray exposure of a radio millisecond pulsar (MSP) to date, an X-ray Multi Mirror-Newton European Photon Imaging Camera spectroscopic and timing observation of the nearest known MSP, PSR J0437--4715. The…

高能天体物理现象 · 物理学 2015-06-12 Slavko Bogdanov

Properties of X-ray radiation emitted from the polar caps of a radio pulsar depend not only on the cap temperature, size, and position, but also on the surface chemical composition, magnetic field, and neutron star's mass and radius.…

天体物理学 · 物理学 2009-10-30 G. G. Pavlov , V. E. Zavlin

We report Bayesian inference of the mass, radius and hot X-ray emitting region properties - using data from the Neutron Star Interior Composition ExploreR (NICER) - for the brightest rotation-powered millisecond X-ray pulsar PSR…

We analyzed the thermal emission from the entire surface of the millisecond pulsar PSR J0437-4715 observed in the ultraviolet and soft X-ray bands. For this, we calculated non-magnetized, partially ionized atmosphere models of hydrogen,…

高能天体物理现象 · 物理学 2020-01-08 Denis Gonzalez-Caniulef , Sebastien Guillot , Andreas Reisenegger

We report on spectral and timing observations of the nearest millisecond pulsar J0437-4715 with Chandra. The pulsar spectrum, detected up to 7 keV, cannot be described by a simple one-component model. We suggest that it consists of two…

天体物理学 · 物理学 2009-11-07 V. E. Zavlin , G. G. Pavlov , D. Sanwal , R. N. Manchester , J. Truemper , J. P. Halpern , W. Becker

We present a multi-wavelength analysis of the nearby millisecond pulsar PSR J0437--4715, combining Hubble Space Telescope (HST) far-ultraviolet, ROSAT soft X-ray, and XMM-Newton X-ray data, to model its broadband emission and…

高能天体物理现象 · 物理学 2026-05-19 Liqiang Qi , Juan Zhang , Weiwei Xu , Shijie Zheng , Mingyu Ge , Ang Li , Shuang-Nan Zhang , Hua Feng , Fangjun Lu

Pulsating thermal X-ray emission from millisecond pulsars can be used to obtain constraints on the neutron star equation of state, but to date only five such sources have been identified. Of these five millisecond pulsars, only two have…

高能天体物理现象 · 物理学 2019-07-17 N. A. Webb , D. Leahy , S. Guillot , N. Baillot d'Etivaux , D. Barret , L. Guillemot , J. Margueron , M. C. Miller

Neutron star Interior Composition Explorer (NICER) data have been used to estimate the masses and radii of the rotation-powered millisecond pulsars PSR J0030$+$0451, PSR J0740$+$6620, PSR J0437$-$4715, PSR J1231$-$1411, and PSR…

I present an analysis of the XMM-Newton observations of four millisecond pulsars, J0437-4715, J2124-3358, J1024-0719, and J0034-0534. The new data provide strong evidence of thermal emission in the X-ray flux detected from the first three…

天体物理学 · 物理学 2010-11-11 Vyacheslav E. Zavlin

Observations of cooling neutron stars allow to measure photospheric radii and to constrain the equation of state of nuclear matter at high densities. In this paper we concentrate on neutron stars, which show thermal (photospheric) X-ray…

天体物理学 · 物理学 2007-05-23 J. E. Truemper

XMM-Newton observations of the middle-aged radio-quiet $\gamma$-ray pulsar J0554+3107 allowed us, for the first time, firmly identify it in X-rays by detection of pulsations with the pulsar period. In the 0.2-2 keV band, the pulse profile…

高能天体物理现象 · 物理学 2023-05-18 A. S. Tanashkin , A. V. Karpova , A. Y. Potekhin , Y. A. Shibanov , D. A. Zyuzin

X-ray emission from many rotation-powered millisecond pulsars (MSPs) is observed to be of predominantly thermal nature. In PSR J0437--4715, the nearest MSP known, an additional faint power-law tail is observed above 2.5 keV, commonly…

天体物理学 · 物理学 2011-02-11 Slavko Bogdanov , Jonathan E. Grindlay , George B. Rybicki

We report results of XMM-Newton observations of a $\gamma$-ray pulsar J0633+0632 and its wind nebula. We reveal, for the first time, pulsations of the pulsar X-ray emission with a single sinusoidal pulse-profile and a pulsed fraction of $23…

高能天体物理现象 · 物理学 2020-03-03 Andrey Danilenko , Anna Karpova , Dmitry Ofengeim , Yury Shibanov , Dmitry Zyuzin

The properties of X-ray radiation from the polar caps predicted by the radio pulsar models depend on the surface chemical composition, magnetic field and star's mass and radius as well as on the cap temperature, size and position. Fitting…

天体物理学 · 物理学 2008-02-03 G. G. Pavlov , V. E. Zavlin

We present a hard X-ray NuSTAR observation of PSR J0437-4715, the nearest millisecond pulsar. The known pulsations at the apparent pulse period ~5.76 ms are detected at energies up to 20 keV. We measure a photon index $\Gamma= 1.65\pm0.24$…

NICER observed several rotation-powered millisecond pulsars to search for or confirm the presence of X-ray pulsations. When broad and sine-like, these pulsations may indicate thermal emission from hot polar caps at the magnetic poles on the…

We report on the XMM-Newton observations of the 143 ms pulsar PSR J0538+2817. We present evidence for the first detections of pulsed X-rays from the source at a frequency which is consistent with the predicted radio frequency. The pulse…

Thermal X-ray radiation from neutron star soft X-ray transients in quiescence provides the strongest constraints on the cooling rates of neutron stars, and thus on the interior composition and properties of matter in the cores of neutron…

天体物理学 · 物理学 2011-02-11 C. O. Heinke , P. G. Jonker , R. Wijnands , R. E. Taam
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