activity
20112025
most citedThe neutron star in HESS J1731-347: CCOs as laboratories to study the equation of state of superdense matter

77 citations · 217 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2025★ 5 cited

X-ray spectroscopy method of white dwarf mass determination in intermediate polars. External systematic uncertainties

V. F. Suleimanov, L. Ducci, V. Doroshenko +1

The masses of white dwarfs (WDs) in intermediate polars (IPs) can be determined from the shape of their hard X-ray spectra. Here we study the importance of all possible systematic…

astro-ph.HE2024★ 1 cited

Examining the evolution of the Supersoft X-ray Source RX J0513.9-6951

A. Tavleev, V. F. Suleimanov, K. Werner +1

Supersoft X-ray sources (SSS) are thought to be accreting white dwarfs (WDs) in close binary systems, with thermonuclear burning on their surfaces. The SSS RX J0513.9-6951 in the L…

astro-ph.HE2024★ 2 cited

Soft X-ray emission from the classical nova AT 2018bej

A. Tavleev, L. Ducci, V. F. Suleimanov +4

Classical novae are known to demonstrate a supersoft X-ray source (SSS) state following outbursts, which is associated with residual thermonuclear burning on the white dwarf (WD) s…

astro-ph.HE2014★ 77 cited

The neutron star in HESS J1731-347: CCOs as laboratories to study the equation of state of superdense matter

D. Klochkov, V. Suleimanov, G. Pühlhofer +3

Context: Central Compact Objects (CCOs) in supernova remnants are isolated thermally emitting neutron stars (NSs). They are most probably characterized by a magnetic field strength…

astro-ph.HE2013★ 44 cited

A non-pulsating neutron star in the supernova remnant HESS J1731-347 / G353.6-0.7 with a carbon atmosphere

D. Klochkov, G. Puehlhofer, V. Suleimanov +3

Context: The CCO candidate in the center of the supernova remnant shell HESS J1731-347 / G353.6-0.7 shows no pulsations and exhibits a blackbody-like X-ray spectrum. If the absence…

astro-ph.SR2012

Constraints of the compactness of the isolated neutron stars via X-ray phase-resolved spectroscopy

V. Hambaryan, V. Suleimanov, R. Neuhaeuser +1

A model with a condensed iron surface and partially ionized hydrogen-thin atmosphere allows us to fit simultaneously the observed general spectral shape and the broad absorption fe…

astro-ph.HE2012★ 35 cited

Radiative properties of magnetic neutron stars with metallic surfaces and thin atmospheres

A. Y. Potekhin, V. F. Suleimanov, M. van Adelsberg +1

The goal of this work is to develop a simple analytic description of the emission properties (spectrum and polarization) of the condensed, strongly magnetized surface of neutron st…

astro-ph.SR2011★ 53 cited

Phase resolved spectroscopic study of the isolated neutron star RBS 1223 (1RXS J130848.6+212708)

V. Hambaryan, V. Suleimanov, A. D. Schwope +3

The data from all observations of RBS 1223 (1RXS J130848.6+212708) conducted by XMM-Newton EPIC pn with the same instrumental setup in 2003-2007 were combined to form spin-phase re…