activity
19972023
most citedThe binary fraction of extreme horizontal branch stars

353 citations · 1.4k across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.SR2023

TIC 378898110: A Bright, Short-Period AM CVn Binary in TESS

Matthew J. Green, J. J. Hermes, Brad N. Barlow +22

AM CVn-type systems are ultracompact, helium-accreting binary systems which are evolutionarily linked to the progenitors of thermonuclear supernovae and are expected to be strong G…

astro-ph.IM2017★ 14 cited

Paving the way to simultaneous multi-wavelength astronomy

M. J. Middleton, P. Casella, P. Gandhi +49

Whilst astronomy as a science is historically founded on observations at optical wavelengths, studying the Universe in other bands has yielded remarkable discoveries, from pulsars…

astro-ph.SR2010★ 18 cited

Spin-resolved spectroscopy of the intermediate polar DQ Her

S. Bloemen, T. R. Marsh, D. Steeghs +1

We present high-speed spectroscopic observations of the intermediate polar DQ Herculis. Doppler tomography of two He I lines reveals a spiral density structure in the accretion dis…

astro-ph2004★ 8 cited

Spiral shock detection on eclipse maps: Simulations and Observations

E. T. Harlaftis, R. Baptista, L. Morales-Rueda +2

We perform simulations in order to reveal the effect of observational and physical parameters on the reconstruction of a spiral structure in an accretion disk, using eclipse mappin…

astro-ph2003★ 116 cited

Optical spectra of the carbon-oxygen accretion discs in the ultra-compact X-ray binaries 4U 0614+09, 4U 1543-624 and 2S 0918-549

G. Nelemans, P. G. Jonker, T. R. Marsh +1

We present optical spectra in the range 4600 -- 8600 A for three low-mass X-ray binaries which have been suggested to belong to the class of ultra-compact X-ray binaries based on t…

astro-ph2002★ 156 cited

Orbital periods of twenty two subdwarf B stars

L. Morales-Rueda, P. F. L. Maxted, T. R. Marsh +2

Subdwarf B (sdB) stars are thought to be core helium burning stars with low mass hydrogen envelopes. In recent years it has become clear that many sdB stars lose their hydrogen thr…