Pablo
Rodríguez Gil
Profesor Titular Universidad
![Foto de Pablo](/img/uploaded/AB42DBD222704EDA38F810F80D86EA4B.jpg)
![Foto de University of Warwick](/img/noimage_org.png)
University of Warwick
Coventry, Reino UnidoPublicacións en colaboración con investigadores/as de University of Warwick (74)
2024
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The donor star radial velocity curve in the cataclysmic variable GY Cnc confirms white dwarf eclipse modelling mass
Monthly Notices of the Royal Astronomical Society, Vol. 527, Núm. 2, pp. 4353-4358
2023
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Systematic uncertainties in the characterization of helium-dominated metal-polluted white dwarf atmospheres
Monthly Notices of the Royal Astronomical Society, Vol. 520, Núm. 2, pp. 2843-2866
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The orbital period of the recurrent nova V2487 Oph revealed
Monthly Notices of the Royal Astronomical Society, Vol. 526, Núm. 4, pp. 4961-4975
2022
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A 62-minute orbital period black widow binary in a wide hierarchical triple
Nature, Vol. 605, Núm. 7908, pp. 41-45
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A Tentative 114 minute Orbital Period Challenges the Ultracompact Nature of the X-Ray Binary 4U 1812-12
Astrophysical Journal Letters, Vol. 931, Núm. 1
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A dense 0.1-solar-mass star in a 51-minute-orbital-period eclipsing binary
Nature, Vol. 610, Núm. 7932, pp. 467-471
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The post-common-envelope binary central star of the planetary nebula Ou 5: A doubly eclipsing post-red-giant-branch system
Monthly Notices of the Royal Astronomical Society, Vol. 510, Núm. 2, pp. 3102-3110
2021
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A transmission spectrum of the planet candidate WD 1856+534 b and a lower limit to its mass
Astronomy and Astrophysics, Vol. 649
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BG Tri: An example of a low-inclination RW Sex-type nova-like
Monthly Notices of the Royal Astronomical Society, Vol. 503, Núm. 1, pp. 1431-1441
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GD 424 - A helium-atmosphere white dwarf with a large amount of trace hydrogen in the process of digesting a rocky planetesimal
Monthly Notices of the Royal Astronomical Society, Vol. 501, Núm. 3, pp. 4276-4288
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HiPERCAM: A quintuple-beam, high-speed optical imager on the 10.4-m Gran Telescopio Canarias
Monthly Notices of the Royal Astronomical Society, Vol. 507, Núm. 1, pp. 350-366
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Velocity-imaging the rapidly precessing planetary disc around the white dwarf HE 1349-2305 using Doppler tomography
Monthly Notices of the Royal Astronomical Society, Vol. 508, Núm. 4, pp. 5657-5670
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White dwarfs with planetary remnants in the era of Gaia - I. Six emission line systems
Monthly Notices of the Royal Astronomical Society, Vol. 504, Núm. 2, pp. 2707-2726
2020
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A Systematic Search of Zwicky Transient Facility Data for Ultracompact Binary LISA-detectable Gravitational-wave Sources
Astrophysical Journal, Vol. 905, Núm. 1
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IGAPS: The merged IPHAS and UVEX optical surveys of the northern Galactic plane
Astronomy and Astrophysics, Vol. 638
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Single magnetic white dwarfs with Balmer emission lines: A small class with consistent physical characteristics as possible signposts for close-in planetary companions
Monthly Notices of the Royal Astronomical Society, Vol. 499, Núm. 2, pp. 2564-2574
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When the disc's away, the stars will play: Dynamical masses in the nova-like variable KR Aur with a pinch of accretion
Monthly Notices of the Royal Astronomical Society, Vol. 494, Núm. 1, pp. 425-441
2019
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A planetesimal orbiting within the debris disc around a white dwarf star
Science, Vol. 364, Núm. 6435, pp. 66-69
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Observatory science with eXTP
Science China: Physics, Mechanics and Astronomy, Vol. 62, Núm. 2
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Phase-resolved spectroscopy of Gaia14aae: Line emission from near the white dwarf surface
Monthly Notices of the Royal Astronomical Society, Vol. 485, Núm. 2, pp. 1947-1960