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20042024
most citedHST/FGS Parallaxes of AM CVn Stars and Astrophysical Consequences

93 citations · 544 across the 17 of their papers we have counts for

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8 papers · 1 filter

astro-ph2008★ 21 cited

Extremely red stellar objects revealed by IPHAS

N. J. Wright, R. Greimel, M. J. Barlow +13

We present photometric analysis and follow-up spectroscopy for a population of extremely red stellar objects extracted from the point-source catalogue of the INT Photometric H-Alph…

astro-ph2007★ 39 cited

Newly Discovered Cataclysmic Variables from the INT/WFC Photometric H alpha Survey of the Northern Galactic Plane

A. R. Witham, C. Knigge, A. Aungwerojwit +7

We report the discovery of 11 new cataclysmic variable (CV) candidates by the Isaac Newton Telescope (INT) Photometric H alpha Survey of the northern Galactic plane (IPHAS). Three…

astro-ph2007★ 93 cited

HST/FGS Parallaxes of AM CVn Stars and Astrophysical Consequences

G. H. A. Roelofs, P. J. Groot, G. F. Benedict +5

We present absolute parallaxes and relative proper motions for five AM CVn stars, which we obtained using the Fine Guidance Sensors on board the Hubble Space Telescope. Our paralla…

astro-ph2007★ 34 cited

DE CVn: A bright, eclipsing red dwarf - white dwarf binary

E. J. M. van den Besselaar, R. Greimel, L. Morales-Rueda +10

Close white dwarf - red dwarf binaries must have gone through a common-envelope phase during their evolution. DE CVn is a detached white dwarf - red dwarf binary with a relatively…

astro-ph2006★ 69 cited

Kinematics of the ultra-compact helium accretor AM Canum Venaticorum

G. H. A. Roelofs, P. J. Groot, G. Nelemans +2

We report on the results from a five-night campaign of high-speed spectroscopy of the 17-minute binary AM Canum Venaticorum, obtained with the 4.2-m William Herschel Telescope on L…

astro-ph2006★ 23 cited

GEMINI spectroscopy of the ultra-compact binary candidate V407 Vul

D. Steeghs, T. R. Marsh, S. C. C. Barros +5

We present time-resolved spectroscopy of the optical counterpart to the proposed ultra-compact binary system V407 Vul (=RX J1914.4+2456). Our Gemini spectra resolve the 9.48 minute…