activity
20092026
most citedA Data Release 2 catalogue of white dwarfs and a comparison with SDSS

424 citations · 3.4k across the 66 of their papers we have counts for

collaborators

66 papers

astro-ph.SR2026

Reframing the Wide Eccentric Binary Problem: Eccentricity as a Probe of Mass-transfer Physics

A. Parkosidis, S. Toonen, E. Laplace +1

Observations of wide post-interaction binaries show an unexpected feature; orbital eccentricity, which is not understood theoretically. A promising resolution to this long-standing…

astro-ph.SR2025

The Silent Majority: The Interacting Post-Common-Envelope Binaries Underlying Cataclysmic Variables

Yarin Meir Shani, Na'ama Hallakoun, Sagi Ben-Ami +4

We analyze the orbital period distribution of post-common-envelope white-dwarf-main-sequence (WDMS) binaries by cross-matching the new spectroscopic Gaia DR3 WDMS catalog with TESS…

astro-ph.SR2025★ 5 cited

Gaia Barium Dwarfs and Their Ostensibly Ordinary Counterparts

Param Rekhi, Sahar Shahaf, Sagi Ben-Ami +4

The recently identified Gaia population of main-sequence--white dwarf (MS+WD) binaries at separations of , often with moderate eccentricities, is not readily re…

astro-ph.SR2025

Tertiary Tides with Eccentric Orbits

Yan Gao, Tjarda Boekholt, Devismita Panda +2

Within hierarchical triple stellar systems, there exists a tidal process unique to them, known as tertiary tides. In this process, the tidal deformation of a tertiary in a hierarch…

astro-ph.SR2025

Eclipsing white dwarf from the Zwicky Transient Facility: II. Seven eclipsing double white dwarfs

J. van Roestel, K. Burdge, I. Caiazzo +15

In a systematic search for eclipsing white dwarfs using Zwicky transient facility (ZTF) data, we found seven eclipsing double white dwarfs with orbital periods ranging from 45 minu…

astro-ph.SR2025★ 4 cited

The role of triple evolution in the formation of LISA double white dwarfs

Abinaya Swaruba Rajamuthukumar, Valeriya Korol, Jakob Stegmann +5

Galactic double white dwarfs will be prominent gravitational-wave sources for the Laser Interferometer Space Antenna (LISA). While previous studies have primarily focused on format…

astro-ph.SR2024

Massive White Dwarfs in the 100 pc Sample: Magnetism, Rotation, Pulsations, and the Merger Fraction

Gracyn Jewett, Mukremin Kilic, Pierre Bergeron +6

We present a detailed model atmosphere analysis of massive white dwarfs with and K in the Montreal White Dwarf Database 100 pc sample and…

astro-ph.SR2024★ 8 cited

Ba Enrichment in Gaia MS+WD Binaries: Tracing -Process Element Production

Param Rekhi, Sagi Ben-Ami, Na'ama Hallakoun +3

A large population of intermediate-separation binaries, consisting of a main-sequence (MS) star and a white dwarf (WD), has recently emerged from Gaia's third data release (DR3), p…

astro-ph.SR2024

The DBL Survey I: discovery of 34 double-lined double white dwarf binaries

James Munday, Ingrid Pelisoli, P. E. Tremblay +8

We present the first discoveries of the double-lined double white dwarf (DBL) survey that targets over-luminous sources with respect to the canonical white dwarf cooling sequence a…

astro-ph.EP2024

White Dwarf Pollution: One Star or Two?

Hiba Tu Noor, Jay Farihi, Mark Hollands +1

The accretion of tidally disrupted planetary bodies is the current consensus model for the presence of photospheric metals commonly detected in white dwarfs. While most dynamical s…

astro-ph.SR2024★ 88 cited

The 40 pc sample of white dwarfs from Gaia

Mairi W. O'Brien, P. -E. Tremblay, B. L. Klein +14

We present a comprehensive overview of a volume-complete sample of white dwarfs located within 40 pc of the Sun, a significant proportion of which were detected in Gaia Data Releas…

astro-ph.SR2023★ 23 cited

A Deficit of Massive White Dwarfs in Gaia Astrometric Binaries

Na'ama Hallakoun, Sahar Shahaf, Tsevi Mazeh +2

The third data release of Gaia introduced a large catalog of astrometric binaries, out of which about 3,200 are likely main-sequence stars with a white-dwarf (WD) companion. These…

astro-ph.EP2023

WD0141-675: A case study on how to follow-up astrometric planet candidates around white dwarfs

Laura K. Rogers, John Debes, Richard J. Anslow +22

This work combines spectroscopic and photometric data of the polluted white dwarf WD0141-675 which has a now retracted astrometric super-Jupiter candidate and investigates the most…

astro-ph.HE2023★ 2 cited

Neutron Star - White Dwarf Binaries: Probing Formation Pathways and Natal Kicks with LISA

Valeriya Korol, Andrei P. Igoshev, Silvia Toonen +4

Neutron star-white dwarf (NS+WD) binaries offer a unique opportunity for studying NS-specific phenomena with gravitational waves. In this paper, we employ the binary population syn…

astro-ph.SR2023★ 4 cited

Triage of the Gaia DR3 astrometric orbits. II. A census of white dwarfs

S. Shahaf, N. Hallakoun, T. Mazeh +4

The third data release of Gaia was the first to include orbital solutions assuming non-single stars. Here, we apply the astrometric triage technique of Shahaf et al. to identify bi…

astro-ph.SR2023★ 46 cited

A massive helium star with a sufficiently strong magnetic field to form a magnetar

T. Shenar, G. A. Wade, P. Marchant +13

Magnetars are highly magnetized neutron stars; their formation mechanism is unknown. Hot helium-rich stars with spectra dominated by emission lines are known as Wolf-Rayet stars. W…

astro-ph.EP2023★ 7 cited

Statistics of Magrathea exoplanets beyond the Main Sequence. Simulating the long-term evolution of circumbinary giant planets with TRES

Gabriele Columba, Camilla Danielski, Andris Dorozsmai +2

Notwithstanding the tremendous growth of the exoplanetary field in the last decade, limited attention has been paid to the planets around binary stars. Circumbinary planets (CBPs)…

astro-ph.SR2022★ 42 cited

The Merger Fraction of Ultramassive White Dwarfs

Mukremin Kilic, Adam G. Moss, Alekzander Kosakowski +6

We search for merger products among the 25 most massive white dwarfs in the Montreal White Dwarf Database 100 pc sample through follow-up spectroscopy and high-cadence photometry.…

astro-ph.SR2022★ 54 cited

white dwarfs within 40 pc III: spectroscopic observations of new candidates in the southern hemisphere

Mairi W. O'Brien, P. -E. Tremblay, N. P. Gentile Fusillo +31

We present a spectroscopic survey of 248 white dwarf candidates within 40 pc of the Sun; of these 244 are in the southern hemisphere. Observations were performed mostly with the Ve…

astro-ph.SR2022★ 28 cited

Local stellar formation history from the 40 pc white dwarf sample

E. Cukanovaite, P. -E. Tremblay, S. Toonen +4

We derive the local stellar formation history from the Gaia-defined 40 pc white dwarf sample. This is currently the largest volume-complete sample of white dwarfs for which spectro…

astro-ph.HE2022★ 34 cited

The origins of Calcium-rich supernovae from disruptions of CO white-dwarfs by hybrid He-CO white-dwarfs

Yossef Zenati, Hagai B. Perets, Luc Dessart +3

Calcium-rich (SN 2005E-like) explosions are very faint (typical -15.5, type I supernovae (SNe) showing strong Ca-lines, mostly observed in old stellar environments. Several models…

astro-ph.SR2022★ 19 cited

Von Zeipel - Lidov - Kozai cycles in action: triples with eclipse depth variations: KICs 6964043, 5653126, 5731312 and 8023317

T. Borkovits, S. A. Rappaport, S. Toonen +3

We report the results of the photodynamical analyses of four compact, tight triple stellar systems, KICs 6964043, 5653126, 5731312, 8023317, based largely on and da…

astro-ph.SR2022★ 4 cited

Importance of stable mass transfer and stellar winds for the formation of gravitational wave sources

Andris Dorozsmai, Silvia Toonen

The large number of gravitational wave (GW) detections have revealed the properties of the merging black hole binary population, but how such systems are formed is still heavily de…

astro-ph.HE2022★ 2 cited

Evidence for Extended Hydrogen-Poor CSM in the Three-Peaked Light Curve of Stripped Envelope Ib Supernova

Yossef Zenati, Qinan Wang, Alexey Bobrick +40

We present multi-band ATLAS photometry for SN 2019tsf, a stripped-envelope Type Ib supernova (SESN). The SN shows a triple-peaked light curve and a late (re-)brightening, making it…