activity
20142026
most citedA radio pulsing white dwarf binary star

215 citations · 1.1k across the 44 of their papers we have counts for

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30 papers · 1 filter

astro-ph.SR2026

Now you see me, now you don't: Deep, long-lived obscuration events of white dwarfs by dust and debris from disintegrating planetesimals

J. van Roestel, S. Bhattacharjee, J. A. Guidry +22

Transiting dust and debris around white dwarfs provide a direct view of planetary disruption. We report six previously non-variable white dwarfs that underwent single, deep obscura…

astro-ph.SR2026

A survey of ultra-compact high-state AM CVn binaries with ZTF and Gaia: New discoveries and observational constraints on Galactic space density

Ilkham Galiullin, Antonio C. Rodriguez, Kareem El-Badry +9

Ultra-compact AM CVn binaries in the high-state of stable mass transfer () are expected to be among the loudest persistent sources for upcomin…

astro-ph.SR2026

V407 Vul: a triple star system with an AM CVn detectable by gravitational wave observatories

James Munday, Antonio C. Rodriguez, Nicole Reindl +23

The AM CVn class includes mass transferring, ultra-compact double white dwarf binaries with orbital periods on the timescale of minutes. A long-standing puzzle is that none of the…

astro-ph.SR2026

No Period Change in Two Long-Period AM CVn Binaries

Matthew J. Green, Thomas R. Marsh, Jan van Roestel +25

Ultracompact binary systems, consisting of two compact objects in an orbit , should exhibit measurable rates of orbital period change () due t…

astro-ph.SR2025

Circumstellar interaction in the extreme white dwarf merger remnant ZTF\,J1901+1458: A new class of white dwarf merger remnants with X-ray emission

Aayush Desai, Ilaria Caiazzo, Stephane Vennes +31

Double degenerate white dwarf (WD) mergers can exhibit extreme magnetic fields exceeding G and rapid rotation, but their spectral-energy distributions and high-energy emis…

astro-ph.SR2025

Variability of Central Stars of Planetary Nebulae with the Zwicky Transient Facility. II. Long-Timescale Variables including Wide Binary and Late Thermal Pulse Candidates

Soumyadeep Bhattacharjee, Nicole Reindl, Howard E. Bond +14

In this second paper on our variability survey of central stars of planetary nebulae (CSPNe) using ZTF, we report 11 long-timescale variables with variability timescales ranging fr…

astro-ph.SR2025

Two almost planetary mass survivors of common envelope evolution

S. G. Parsons, A. J. Brown, S. L. Casewell +19

White dwarfs are often found in close binaries with stellar or even substellar companions. It is generally thought that these compact binaries form via common envelope evolution, t…

astro-ph.SR2024

A gravitational wave detectable candidate Type Ia supernova progenitor

Emma T. Chickles, Kevin B. Burdge, Joheen Chakraborty +37

Type Ia supernovae, critical for studying cosmic expansion, arise from thermonuclear explosions of white dwarfs, but their precise progenitor pathways remain unclear. Growing evide…

astro-ph.SR2024★ 2 cited

Hertzsprung gap stars in nearby galaxies and the Quest for Luminous Red Novae Progenitors

Hugo Tranin, Nadejda Blagorodnova, Viraj Karambelkar +5

After the main sequence phase, stars more massive than 2.5 M rapidly evolve through the Hertzsprung gap as yellow giants and supergiants (YSG), before settling into the red…

astro-ph.SR2023

A systematic search for double eclipsing binaries in Zwicky Transient Facility data

T. Vaessen, J. van Roestel

Context. Double eclipsing binaries are gravitationally bound quadruple systems in a 2+2 configuration where both of the binaries are eclipsing. These systems are interesting object…

astro-ph.SR2023

OGLE-BLAP-009 -- A Case Study for the Properties and Evolution of Blue Large-Amplitude Pulsators

Corey W. Bradshaw, Matti Dorsch, Thomas Kupfer +5

Blue large-amplitude pulsators (BLAPs) make up a rare class of hot pulsating stars with effective temperatures of 30,000 K and surface gravities of 4.0 - 5.0 dex (cgs). Th…

astro-ph.SR2023★ 26 cited

Period bouncers as detached magnetic cataclysmic variables

Matthias R. Schreiber, Diogo Belloni, Jan van Roestel

The general prediction that more than half of all CVs have evolved past the period minimum is in strong disagreement with observational surveys, which show that the relative number…

astro-ph.SR2023

RNO 54: A Previously Unappreciated FU Ori Star

Lynne A. Hillenbrand, Adolfo Carvalho, Jan van Roestel +1

We present evidence in support of the hypothesis that the young stellar object RNO 54 is a mature-stage FU Ori type source. The star was first cataloged as a ``red nebulous object"…

astro-ph.SR2023

An Extremely Massive White Dwarf Escaped From the Hyades Star Cluster

David R. Miller, Ilaria Caiazzo, Jeremy Heyl +5

We searched the Gaia DR3 database for ultramassive white dwarfs with kinematics consistent with having escaped the nearby Hyades open cluster, identifying three such candidates. Tw…

astro-ph.SR2023★ 27 cited

A transiting brown dwarf in a 2 hour orbit

Kareem El-Badry, Kevin B. Burdge, Jan van Roestel +1

We report the discovery of ZTF J2020+5033, a high-mass brown dwarf (BD) transiting a low-mass star with an orbital period of 1.90 hours. Phase-resolved spectroscopy, optical and in…

astro-ph.SR2023★ 15 cited

Spectroscopic follow-up of black hole and neutron star candidates in ellipsoidal variables from Gaia DR3

Pranav Nagarajan, Kareem El-Badry, Antonio C. Rodriguez +2

We present multi-epoch spectroscopic follow-up of a sample of ellipsoidal variables selected from Gaia DR3 as candidates for hosting quiescent black holes (BHs) and neutron stars (…

astro-ph.SR2023★ 17 cited

Orbital decay in an accreting and eclipsing 13.7 minute orbital period binary with a luminous donor

Kevin B. Burdge, Kareem El-Badry, Saul Rappaport +24

We report the discovery of ZTF J0127+5258, a compact mass-transferring binary with an orbital period of 13.7 minutes. The system contains a white dwarf accretor, which likely origi…

astro-ph.SR2023★ 22 cited

Photometric follow-up of 43 new eclipsing white dwarf plus main-sequence binaries from the ZTF survey

Alex J. Brown, Steven G. Parsons, Jan van Roestel +12

Wide-field time-domain photometric sky surveys are now finding hundreds of eclipsing white dwarf plus M dwarf binaries, a population encompassing a wealth of information and potent…

astro-ph.SR2022★ 51 cited

Magnetic braking saturates: evidence from the orbital period distribution of low-mass detached eclipsing binaries from ZTF

Kareem El-Badry, Charlie Conroy, Jim Fuller +4

We constrain the orbital period () distribution of low-mass detached main-sequence eclipsing binaries (EBs) with light curves from the Zwicky Transient Facility (ZTF),…

astro-ph.SR2021★ 106 cited

A WC/WO star exploding within an expanding carbon-oxygen-neon nebula

A. Gal-Yam, R. Bruch, S. Schulze +46

The final explosive fate of massive stars, and the nature of the compact remnants they leave behind (black holes and neutron stars), are major open questions in astrophysics. Many…

astro-ph.SR2021★ 38 cited

Discovery of a double detonation thermonuclear supernova progenitor

Thomas Kupfer, Evan B. Bauer, Jan van Roestel +12

We present the discovery of a new double detonation progenitor system consisting of a hot subdwarf B (sdB) binary with a white dwarf companion with an P=76.34179(2) min orbital per…

astro-ph.SR2021★ 16 cited

Cataclysmic Variables in the Second Year of the Zwicky Transient Facility

Paula Szkody, Clair Olde Loohuis, Brad Koplitz +17

Using a filter in the GROWTH Marshal based on color and the amplitude and the timescale of variability, we have identified 372 objects as known or candidate cataclysmic variables (…

astro-ph.SR2021★ 15 cited

Confirmation of a Second Propeller: A High-Inclination Twin of AE~Aquarii

Peter Garnavich, Colin Littlefield, R. M. Wagner +4

For decades, AE Aquarii (AE Aqr) has been the only cataclysmic variable star known to contain a magnetic propeller: a persistent outflow whose expulsion from the binary is powered…

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…