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19942026
most citedA Massive Pulsar in a Compact Relativistic Binary

3.9k citations

Showing 2019 · astro-ph.HEShow all

12 papers · 2 filters

astro-ph.HE2019★ 26 cited

Coronal properties of black hole X-ray binaries in the hard state as seen by NuSTAR and Swift

Zhen Yan, Fu-guo Xie, Wenda Zhang

In this work, we measure two important phenomenological parameters of corona (and hot accretion flow) in black hole X-ray binaries: the photon index and the electron temperatur…

astro-ph.HE2019★ 17 cited

An Oppositeness in the Cosmology: Distribution of the Gamma-Ray Bursts and the Cosmological Principle

Attila Meszaros

The Cosmological Principle is the assumption that the universe is spatially homogeneous and isotropic in the large-scale average. In year 1998 the author, together with his two col…

astro-ph.HE2019★ 146 cited

A NICER view of PSR J0030+0451: evidence for a global-scale multipolar magnetic field

Anna V. Bilous, Anna L. Watts, Alice K. Harding +8

Recent modeling of NICER observations of thermal X-ray pulsations from the surface of the isolated millisecond pulsar PSR J0030+0451 suggests that the hot emitting regions on the p…

astro-ph.HE2019★ 272 cited

A NICER view of PSR J0030+0451: Implications for the dense matter equation of state

G. Raaijmakers, T. E. Riley, A. L. Watts +14

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 NICER mission. In this Letter we st…

astro-ph.HE2019★ 1.7k cited

A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation

Thomas E. Riley, Anna L. Watts, Slavko Bogdanov +13

We report on Bayesian parameter estimation of the mass and equatorial radius of the millisecond pulsar PSR J00300451, conditional on pulse-profile modeling of Neutron Star Inter…

astro-ph.HE2019★ 12 cited

Low-frequency radio absorption in Tycho's supernova remnant

Maria Arias, Jacco Vink, Ping Zhou +3

Tycho's SNR is the remnant of the type Ia supernova explosion SN1572. In this work we present new low-frequency radio observations with the LOFAR Low-Band and High-Band Antennae, c…

astro-ph.HE2019★ 18 cited

Optical, J, and K light curves of XTE J1118+480 = KV UMa: the mass of the black hole and the spectrum of the non-stellar component

A. M. Cherepashchuk, N. A. Katysheva, T. S. Khruzina +3

Optical, J, and K photometric observations of the KV UMa black hole X-ray nova in its quiescent state obtained in 2017-2018 are presented. A significant flickering within light cur…

astro-ph.HE2019★ 31 cited

Rapidly evolving disk-jet coupling during re-brightenings in the black hole transient MAXI J1535-571

A. S. Parikh, T. D. Russell, R. Wijnands +3

The main outburst of the candidate black hole low-mass X-ray binary (BH LMXB) MAXI J1535-571 ended in 2018 May and was followed by at least five episodes of re-brightenings. We hav…

astro-ph.HE2019★ 24 cited

Ultraluminous X-ray sources with flat-topped noise and QPO

K. Atapin, S. Fabrika, M. D. Caballero-Garcia

We analyzed the X-ray power density spectra of five ultraluminous X-ray sources (ULXs) NGC5408 X-1, NGC6946 X-1, M82 X-1, NGC1313 X-1 and IC342 X-1 that are the only ULXs which dis…

astro-ph.HE2019★ 76 cited

Constraining the size of the corona with fully relativistic calculations of spectra of extended corona. I - the Monte Carlo radiative transfer code

Wenda Zhang, Michal Dovčiak, Michal Bursa

The size and geometry of the X-ray emitting corona in AGNs are still not well constrained. Dovčiak & Done (2016) proposed a method based on calculations assuming a point-like lamp-…

astro-ph.HE2019★ 4 cited

Electromagnetic Window into the Dawn of Black Holes

Zoltán Haiman, William N. Brandt, Alexey Vikhlinin +28

Massive 10^6-10^10 Msun black holes (BHs) are ubiquitous in local galactic nuclei. They were common by the time the Universe is several Gyr old, and many of them were in place with…

astro-ph.HE2019★ 161 cited

A sample of low energy bursts from FRB 121102

K. Gourdji, D. Michilli, L. G. Spitler +4

We present 41 bursts from the first repeating fast radio burst discovered (FRB 121102). A deep search has allowed us to probe unprecedentedly low burst energies during two consecut…