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19952023
most citedA Massive Pulsar in a Compact Relativistic Binary

3.9k citations · 18.7k across the 302 of their papers we have counts for

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Showing 2019Show all

14 papers · 1 filter

astro-ph.HE2019★ 43 cited

A Black Hole X-ray Binary at 100 Hz: Multiwavelength Timing of MAXI J1820+070 with HiPERCAM and NICER

J. A. Paice, P. Gandhi, T. Shahbaz +12

We report on simultaneous sub-second optical and X-ray timing observations of the low mass X-ray binary black hole candidate MAXI J1820+070. The bright 2018 outburst rise allowed s…

astro-ph.EP2019★ 22 cited

Doppler tomography as a tool for detecting exoplanet atmospheres

Christopher Watson, Ernst de Mooij, Danny Steeghs +4

High-resolution Doppler spectroscopy is a powerful tool for identifying molecular species in the atmospheres of both transiting and non-transiting exoplanets. Currently, such data…

astro-ph.SR2019★ 155 cited

Core crystallization and pile-up in the cooling sequence of evolving white dwarfs

Pier-Emmanuel Tremblay, Gilles Fontaine, Nicola Pietro Gentile Fusillo +7

White dwarfs are stellar embers depleted of nuclear energy sources that cool over billions of years. These stars, which are supported by electron degeneracy pressure, reach densiti…

astro-ph.SR2019★ 52 cited

The EREBOS project -- Investigating the effect of substellar and low-mass stellar companions on late stellar evolution

V. Schaffenroth, B. N. Barlow, S. Geier +14

Eclipsing post-common envelope binaries are highly important for resolving the poorly understood, very short-lived common envelope phase. Most hot subdwarfs (sdO/Bs) are the bare H…

astro-ph.SR2019★ 9 cited

Short period variable stars in young open cluster Stock 8

Sneh Lata, Anil. K. Pandey, Ram Kesh Yadav +5

We present time series photometry in the field of Stock 8 and identified 130 short period variable stars. Twenty eight main-sequence and 23 pre-main-sequence variables are found to…

astro-ph.HE2019★ 15 cited

Optical and X-ray Correlations During the 2015 Outburst of the Black Hole V404 Cyg

R. I. Hynes, E. L. Robinson, D. M. Terndrup +5

We present a serendipitous multiwavelength campaign of optical photometry simultaneous with Integral X-ray monitoring of the 2015 outburst of the black hole V404 Cyg. Large amplitu…

astro-ph.EP2019★ 169 cited

A planetesimal orbiting within the debris disc around a white dwarf star

Christopher J. Manser, Boris T. Gänsicke, Siegfried Eggl +29

Many white dwarf stars show signs of having accreted smaller bodies, implying that they may host planetary systems. A small number of these systems contain gaseous debris discs, vi…

astro-ph.SR2019★ 82 cited

The evolutionary status of Cataclysmic Variables: Eclipse modelling of 15 systems

M. McAllister, S. P. Littlefair, S. G. Parsons +13

We present measurements of the component masses in 15 Cataclysmic Variables (CVs) - 6 new estimates and 9 improved estimates. We provide new calibrations of the relationship betwee…

astro-ph.SR2019★ 4 cited

Astro2020 Science White Paper: Understanding the evolution of close white dwarf binaries

Odette Toloza, Elme Breed, Domitilla De Martino +27

Interacting binaries containing white dwarfs can lead to a variety of outcomes that range from powerful thermonuclear explosions, which are important in the chemical evolution of g…

astro-ph.HE2019

Multimessenger science opportunities with mHz gravitational waves

John Baker, Zoltán Haiman, Elena Maria Rossi +32

LISA will open the mHz band of gravitational waves (GWs) to the astronomy community. The strong gravity which powers the variety of GW sources in this band is also crucial in a num…

astro-ph.SR2019

Accurate mass and radius determinations of a cool subdwarf in an eclipsing binary

Alberto Rebassa-Mansergas, Steven G. Parsons, Vikram S. Dhillon +4

Cool subdwarfs are metal-poor low-mass stars that formed during the early stages of the evolution of our Galaxy. Because they are relatively rare in the vicinity of the Sun, we kno…

astro-ph.EP2019★ 47 cited

Pluto's lower atmosphere and pressure evolution from ground-based stellar occultations, 1988-2016

E. Meza, B. Sicardy, M. Assafin +167

Context. Pluto's tenuous nitrogen (N2) atmosphere undergoes strong seasonal effects due to high obliquity and orbital eccentricity, and has been recently (July 2015) observed by th…

astro-ph.SR2019★ 16 cited

Phase-Resolved Spectroscopy of Gaia14aae: Line Emission From Near the White Dwarf Surface

M. J. Green, T. R. Marsh, D. Steeghs +8

AM CVn binaries are a class of ultracompact, hydrogen-deficient binaries, each consisting of a white dwarf accreting helium-dominated material from a degenerate or semi-degenerate…

astro-ph.SR2019★ 12 cited

Evidence for bimodal orbital separations of white dwarf-red dwarf binary stars

R. P. Ashley, J. Farihi, T. R. Marsh +2

We present the results of a radial velocity survey of 20 white dwarf plus M dwarf binaries selected as a follow up to a \textit{Hubble Space Telescope} study that aimed to spatiall…