activity
20202026
most citedA proto-helium white dwarf stripped by a substellar companion via common-envelope ejection -- Uncovering the true nature of a candidate hypervelocity B-type star

36 citations · 94 across the 45 of their papers we have counts for

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Showing 2025Show all

20 papers · 1 filter

astro-ph.HE2025

Search for Radio Pulsations from Neutron Star Candidates in Detached Binaries

Shi-Jie Gao, Xiang-Dong Li, Song Wang +7

Recent optical astrometric and spectroscopic surveys have identified numerous neutron star (NS) candidates in non-accreting detached binary systems, but their compact-object nature…

astro-ph.SR2025

The White Dwarf Initial-Final Mass Relation from Open Clusters in Gaia DR3

David R. Miller, Ilaria Caiazzo, Jeremy Heyl +6

The initial-final mass relation (IFMR) links a star's birth mass to the mass of its white dwarf (WD) remnant, providing key constraints on stellar evolution. Open clusters offer th…

astro-ph.SR2025

A search for black holes with metal-poor stellar companions: I. Survey sample selection and single epoch radial velocity follow-up

Casey Y. Lam, Joshua D. Simon, Kareem El-Badry +3

Stellar-mass black holes (BHs) above are predicted to form from low-metallicity progenitors, but direct detections of such systems in the Milky Way remain scarce. Moti…

astro-ph.SR2025★ 2 cited

Modelling the Future of Gaia Neutron Star-Main Sequence Binaries: From Eccentric Orbits to Millisecond Pulsar-White Dwarfs

Debatri Chattopadhyay, Kyle A. Rocha, Seth Gossage +3

We model the evolution of 21 Gaia neutron star (NS)-main-sequence binaries (orbital period -- days, eccentricity ) using binary evolutio…

astro-ph.SR2025

Intermediate-Mass Stripped Stars in the Magellanic Clouds: Forward Modeling the Observed Population Discovered Via UV Excess

Lisa Blomberg, Kareem El-Badry, Bethany Ludwig +2

Stripped stars are hot, helium-rich stars formed when binary interactions remove a star's hydrogen envelope. While low-mass () and high-mass ($\gtrsim 8 M_\odot…

astro-ph.SR2025★ 2 cited

How precisely can we measure the ages of subgiant and giant stars?

Cheyanne Shariat, Kareem El-Badry, Soumyadeep Bhattacharjee

Precise stellar ages are fundamental to Galactic archaeology. However, obtaining reliable age estimates and uncertainties for field stars has been a long-standing challenge. We tes…

astro-ph.GA2025

Wide binaries in an ultra-faint dwarf galaxy: discovery, population modeling, and a nail in the coffin of primordial black hole dark matter

Cheyanne Shariat, Kareem El-Badry, Mario Gennaro +24

We report the discovery and characterization of a wide binary population in the ultrafaint dwarf galaxy Boötes I using deep JWST/NIRCam imaging. Our sample consists of 52 candidate…

astro-ph.SR2025

Searching for Ultra-light Dark Matter in Spatial Correlations of White Dwarf Structure

Nicole R. Crumpler, Nadia L. Zakamska, Gautham Adamane Pallathadka +1

If dark matter is ultra-light and has certain Standard Model interactions, it can change the mass-radius relation of white dwarf stars. The coherence length of ultra-light dark mat…

astro-ph.SR2025

Double White Dwarf Binaries in SDSS-V DR19 : A catalog of DA white dwarf binaries and constraints on the binary population

Gautham Adamane Pallathadka, Vedant Chandra, Nadia L. Zakamska +17

The fifth-generation Sloan Digital Sky Survey (SDSS-V) includes the first large-scale spectroscopic survey of white dwarfs (WDs) in the era of Gaia parallaxes. SDSS-V collects mult…

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★ 1 cited

Optical Spectroscopy of the Most Compact Accreting Binary Harboring a Magnetic White Dwarf and a Hydrogen-rich Donor

Ilkham Galiullin, Antonio C. Rodriguez, Kareem El-Badry +4

Accreting white dwarfs in close binary systems, commonly known as cataclysmic variables (CVs), with orbital periods below the canonical period minimum ( 80 minutes) are ra…

astro-ph.SR2025★ 1 cited

Transiting Planetary Debris near the Roche Limit of a White Dwarf on a 4.97hr Orbit -- and its Vanishing

Joseph A. Guidry, Zachary P. Vanderbosch, J. J. Hermes +9

We present the discovery of deep, irregular, periodic transits towards the white dwarf ZTFJ19444557 using follow-up time-series photometry and spectroscopy from Palomar, Kec…

astro-ph.SR2025★ 1 cited

Resolution-Corrected White Dwarf Gravitational Redshifts Validate SDSS-V Wavelength Calibration and Enable Accurate Mass-Radius Tests

Stefan M. Arseneau, J. J. Hermes, Nadia L. Zakamska +7

Leveraging the large sample size of low-resolution spectroscopic surveys to constrain white dwarf stellar structure requires an accurate understanding of the shapes of hydrogen abs…

astro-ph.SR2025★ 4 cited

A half-ring of ionized circumstellar material trapped in the magnetosphere of a white dwarf merger remnant

Andrei A. Cristea, Ilaria Caiazzo, Tim Cunningham +31

Many white dwarfs are observed in compact double white dwarf binaries and, through the emission of gravitational waves, a large fraction are destined to merge. The merger remnants…

astro-ph.IM2025★ 3 cited

Sloan Digital Sky Survey-V: Pioneering Panoptic Spectroscopy

Juna A. Kollmeier, Hans-Walter Rix, Conny Aerts +217

The Sloan Digital Sky Survey-V (SDSS-V) is pioneering panoptic spectroscopy: it is the first all-sky, multi-epoch, optical-to-infrared spectroscopic survey. SDSS-V is mapping the s…

astro-ph.SR2025

Carbon burning cannot explain puffy hypervelocity white dwarfs

Natsuko Yamaguchi, Kareem El-Badry, Tin Long Sunny Wong +1

Several hypervelocity white dwarfs (HVWDs) with space velocities of have recently been discovered. One possible origin of these stars is the dynam…

astro-ph.SR2025★ 20 cited

10,000 Resolved Triples from Gaia: Empirical Constraints on Triple Star Populations

Cheyanne Shariat, Kareem El-Badry, Smadar Naoz

We present a catalog of resolved triple star systems within 500 pc of the Sun, constructed using Gaia data. The triples include main-sequence, red giant, and white dw…

astro-ph.SR2025★ 2 cited

Calibration of Binary Population Synthesis Models Using White Dwarf Binaries from APOGEE, GALEX and Gaia

A. C. Rubio, K. Breivik, C. Badenes +5

The effectiveness and stability of mass transfer in binaries system are crucial in determining its final product. Rapid binary population synthesis (BPS) codes simplify the complex…

astro-ph.GA2025★ 2 cited

Hypervelocity Stars Trace a Supermassive Black Hole in the Large Magellanic Cloud

Jiwon Jesse Han, Kareem El-Badry, Scott Lucchini +5

Hypervelocity stars (HVSs) are produced by the Hills mechanism when a stellar binary is disrupted by a supermassive black hole (SMBH). The HVS Survey detected 21 unbound B-type mai…

astro-ph.SR2025★ 10 cited

Cataclysmic Variables in Triples: Formation Models and New Discoveries

Cheyanne Shariat, Kareem El-Badry, Smadar Naoz +2

The formation of cataclysmic variables (CVs) has long been modeled as a product of common envelope evolution (CEE) in isolated binaries. However, a significant fraction of intermed…