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The influence of accretion geometry on the spectral evolution during thermonuclear (type I) X-ray bursts

The effect of accretion on the measurement of neutron star mass and radius in the low-mass X-ray binary 4U 1608-52

The influence of accretion geometry on the spectral evolution during thermonuclear (type I) X-ray bursts

The effect of accretion on the measurement of neutron star mass and radius in the low-mass X-ray binary 4U 1608-52

Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra is M = 1.9±0.3 M ⊙ , the distance is 5.1 < D/ kpc < 6.2, and the hydrogen mass fraction is X < 0.09.

The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

Basic parameters of the helium-accreting X-ray bursting neutron star in 4U 1820-30

Репрезентация геомифологии посредством мифологизированных топонимов носителями сэлишских языков

A dichotomy between the hard state spectral properties of black hole and neutron star X-ray binaries

Completing characterization of photon orbits in Kerr and Kerr-Newman metrics

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