activity
19972025
most citedBinary Star Origin of High Field Magnetic White Dwarfs

231 citations · 1.9k across the 41 of their papers we have counts for

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19 papers · 1 filter

astro-ph2008★ 13 cited

VV Pup in a low state: secondary-star irradiation or stellar activity?

Elena Mason, Steve B. Howell, Travis Barman +2

Aims. Emission lines in polars show complex profiles with multiple components that are typically ascribed to the accretion stream, threading region, accretion spot, and the irradia…

astro-ph2008★ 49 cited

Origin and evolution of magnetars

Lilia Ferrario, D. T. Wickramasinghe

We present a population synthesis study of the observed properties of the magnetars, which allows for X-ray selection effects, investigating the hypothesis that they are drawn from…

astro-ph2008★ 231 cited

Binary Star Origin of High Field Magnetic White Dwarfs

C. A. Tout, D. T. Wickramasinghe, J. Liebert +2

White dwarfs with surface magnetic fields in excess of MG are found as isolated single stars and relatively more often in magnetic cataclysmic variables. Some 1,253 white dwarf…

astro-ph2007★ 56 cited

The birth properties of Galactic millisecond radio pulsars

Lilia Ferrario, Dayal Wickramasinghe

We model the population characteristics of the sample of millisecond pulsars within a distance of 1.5kpc.We find that for a braking index n=3, the birth magnetic field distribution…

astro-ph2006★ 10 cited

High resolution spectra of bright central stars of bipolar planetary nebulae, and the question of magnetic shaping

T. -H. Lee, L. Stanghellini, L. Ferrario +1

We present ESO NTT high resolution echelle spectroscopy of the central stars (CSs) of eight southern bipolar planetary nebulae (PNe) selected for their asymmetry. Our aim was to de…

astro-ph2006★ 181 cited

Spectropolarimetric Survey of Hydrogen-rich White Dwarf Stars

A. Kawka, S. Vennes, G. D. Schmidt +2

We have conducted a survey of 61 southern white dwarfs searching for magnetic fields using Zeeman spectropolarimetry. Our objective is to obtain a magnetic field distribution for t…

astro-ph2006★ 172 cited

Modelling of isolated radio pulsars and magnetars on the fossil field hypothesis

Lilia Ferrario, Dayal Wickramasinghe

We explore the hypothesis that the magnetic fields of neutron stars are of fossil origin. For parametrised models of the distribution of magnetic flux on the Main Sequence and of t…

astro-ph2005

Time dependent non-LTE calculations of ionisation in the early universe

R. Wehrse, D. T. Wickramasinghe, Romeel Davé

We present a new implicit numerical algorithm for the calculation of the time dependent non-Local Thermodynamic Equilibrium of a gas in an external radiation field that is accurate…

astro-ph2005★ 116 cited

The open cluster initial-final mass relationship and the high-mass tail of the white dwarf distribution

L. Ferrario, D. Wickramasinghe, J. Liebert +1

Recent studies of white dwarfs in open clusters have provided new constraints on the initial - final mass relationship (IFMR) for main sequence stars with masses in the range 2.5 -…

astro-ph2001

Could Edge-Lit Type Ia Supernovae be Standard Candles

Eniko Regos, Christopher A. Tout, Dayal Wickramasinghe +2

The progenitors of Type Ia supernovae (SNe Ia) have not been identified. Though they are no longer fashionable we investigate the consequences if a significant number of SNe Ia wer…

astro-ph2001★ 35 cited

Studies of Magnetic and Suspected-Magnetic Southern White Dwarfs

G. D. Schmidt, S. Vennes, D. T. Wickramasinghe +1

Optical spectrophotometry and circular spectropolarimetry are presented for several candidate magnetic white dwarfs that were identified during the Hamburg/ESO survey for bright QS…

astro-ph2000★ 20 cited

The Cyclotron Fundamental Exposed in the High-Field Magnetic Variable V884 Her

G. D. Schmidt, L. Ferrario, D. T. Wickramasinghe +1

High-quality phase-resolved optical spectropolarimetry is presented for the magnetic cataclysmic variable V884 Her. The overall circular polarization during active accretion states…

astro-ph2000★ 48 cited

Type Ia Supernovae and Remnant Neutron Stars

A. R. King, J. E. Pringle, D. T. Wickramasinghe

On the basis of the current observational evidence, we put forward the case that the merger of two CO white dwarfs produces both a Type Ia supernova explosion and a stellar remnant…

astro-ph2000★ 57 cited

WD1953-011 - a magnetic white dwarf with peculiar field structure

P. F. L. Maxted, L. Ferrario, T. R. Marsh +1

We present H-alpha spectra of the magnetic white dwarf star WD1953-011 which confirm the presence of the broad Zeeman components corresponding to a field strength of about 500kG fo…

astro-ph2000★ 22 cited

Eccentric discs in binaries with intermediate mass ratios: Superhumps in the VY Sculptoris stars

J. R. Murray, B. Warner, D. T. Wickramasinghe

We investigate the role of the eccentric disc resonance in systems with mass ratios q greater than 1/4, and demonstrate the effects that changes in the mass flux from the secondary…

astro-ph1999★ 19 cited

Thermal Instability and Evaporation of Accretion Disc Atmospheres

Martijn de Kool, Dayal T. Wickramasinghe

We investigate the thermal stability of the outer layers of accretion discs in which the local viscous energy dissipation rate scales with the pressure as for standard Shakura-Suny…

astro-ph1998★ 15 cited

The effects of tidally induced disc structure on white dwarf accretion in intermediate polars

J. R. Murray, P. J. Armitage, L. Ferrario +1

We investigate the effects of tidally induced asymmetric disc structure on accretion onto the white dwarf in intermediate polars. Using numerical simulation, we show that it is pos…

astro-ph1998★ 38 cited

Measuring the Motion of the Black Hole in GRO J16550-40

Roberto Soria, Dayal T. Wickramasinghe, Richard W. Hunstead +1

We report optical spectroscopic observations of the Low Mass X-ray Binary GRO J1655-40 during outbursts in August-September 1994 and in June 1996. The spectra show emission and abs…

astro-ph1997★ 119 cited

Understanding the Cool DA White Dwarf, G29-38

S. J. Kleinman, R. E. Nather, D. E. Winget +37

The white dwarfs are promising laboratories for the study of cosmochronology and stellar evolution. Through observations of the pulsating white dwarfs, we can measure their interna…