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19952026
most citedThe Evolution of Compact Binary Star Systems

491 citations · 5.1k across the 187 of their papers we have counts for

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Showing 2012Show all

6 papers · 1 filter

astro-ph.HE2012★ 40 cited

Variable pulse profiles of Her X-1 repeating with the same irregular 35d clock as the turn-ons

R. Staubert, D. Klochkov, D. Vasco +4

The accreting X-ray pulsar Her X-1 shows two types of long-term variations, both with periods of ~35 days: 1) Turn-on cycles, a modulation of the flux}, with a ten-day long Main-On…

astro-ph.HE2012★ 1 cited

Peculiarities in the orbital and precessional variability of SS433 from INTEGRAL observations

A. Cherepashchuk, R. Sunyaev, S. Molkov +3

Based on multiyear INTEGRAL observations of SS433, a composite IBIS/ISGRI 18-60 keV orbital light curve is constructed around zero precessional phase . It shows a peculi…

astro-ph.HE2012

Quasi-spherical accretion in low-luminosity X-ray pulsars: Theory vs. observations

K. Postnov, N. Shakura, A. Kochetkova +1

Quasi-spherical subsonic accretion can be realized in slowly rotating wind-fed X-ray pulsars (XPSRs) at X-ray luminosities <4 10^{36} erg/s. In this regime the accreting matter set…

astro-ph.HE2012★ 48 cited

On the nature of `off' states in slowly rotating low-luminosity X-ray pulsars

N. Shakura, K. Postnov, L. Hjalmarsdotter

We elaborate on a recently proposed model for subsonic quasi-spherical accretion onto slowly rotating pulsars, in which accretion is mediated through a hot quasi-static shell above…

astro-ph.SR2012★ 56 cited

Population Synthesis for Symbiotic X-ray Binaries

G. -L. Lu, C. -H. Zhu, K. A. Postnov +3

Symbiotic X-ray binaries (SyXBs) comprise a rare class of low-mass X-ray binaries. We study the Galactic SyXBs, which we consider as detached binaries composed of low-mass giants a…

astro-ph.SR2012

Spin period evolution of the X-ray pulsar GX 1+4

A. González-Galán, E. Kuulkers, P. Kretschmar +4

We report on the long-term evolution of the spin period of the symbiotic X-ray pulsar GX 1+4 and a possible interpretation within a model of quasi-spherical accretion. New period m…