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19952026
most citedA Massive Pulsar in a Compact Relativistic Binary

3.9k citations · 14.3k across the 253 of their papers we have counts for

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Showing 2007Show all

10 papers · 1 filter

astro-ph2007★ 5 cited

Bowen blend echo-tomography of low mass X-ray binaries

T. Muñoz-Darias, I. G. Martinez-Pais, J. Casares +7

We present simultaneous high time resolution (1-10 Hz) X-ray and optical observations of the persistent LMXBs Sco X-1 and V801 Ara(=4U 1636-536). In the case of Sco X-1 we find tha…

astro-ph2007★ 16 cited

A multicolor near-infrared study of the dwarf nova IP Peg

T. Ribeiro, R. Baptista, E. T. Harlaftis +2

We report the analysis of light curves of the eclipsing dwarf nova IP Peg in quiescence. The light curves are dominated by the ellipsoidal variation of the mass-donor sta…

astro-ph2007★ 41 cited

Roche tomography of cataclysmic variables - IV. Starspots and slingshot prominences on BV Cen

C. A. Watson, D. Steeghs, T. Shahbaz +1

We present Roche tomograms of the G5-G8 IV/V secondary star in the long-period cataclysmic variable BV Cen reconstructed from MIKE echelle data taken on the Magellan Clay 6.5-m tel…

astro-ph2007★ 91 cited

The binary properties of the pulsating subdwarf B eclipsing binary PG 1336-018 (NY Vir)

M. Vučković, C. Aerts, R. Østensen +5

We present an unbiased orbit solution and mass determination of the components of the eclipsing binary NY Vir as a critical test for the formation scenarios of subdwarf B stars. We…

astro-ph2007★ 8 cited

Outbursts of EX Hydrae Revisited

N. Mhlahlo, D. A. H. Buckley, V. Dhillon +3

We present optical spectroscopy of EX Hya during its 1991 outburst. This outburst is characterised by strong irradiation of the front face of the secondary star by the white dwarf,…

astro-ph2007★ 30 cited

Echoes from the companion star in Sco X-1

T. Muñoz-Darias, I. G. Martinez-Pais, J. Casares +5

We present simultaneous X-ray (RXTE) and optical (ULTRACAM) narrow band (Bowen blend/HeII and nearby continuum) observations of Sco X-1 at 2-10 Hz time resolution. We find that the…