activity
20242026
collaborators

8 papers

astro-ph.SR2026

Spectroscopic follow-up of compact object binary candidates from Gaia DR3: White dwarfs, neutron stars, black holes, and the parallax zeropoint

Kareem El-Badry, David W. Latham, Hans-Walter Rix +12

Astrometry and radial velocities (RVs) from Gaia DR3 yielded orbits for hundreds of thousands of binary systems, including several samples proposed to contain black holes (BHs), ne…

astro-ph.SR2026

Population demographics of post-interaction WDMS binaries: From common envelope evolution to stable mass transfer

Natsuko Yamaguchi, Kareem El-Badry, Cheyanne Shariat

Close white dwarf (WD) + main-sequence (MS) binaries are end products of mass transfer (MT) that occurred when the WD progenitor was a giant, making their population demographics a…

astro-ph.SR2026

A systematic survey for hypervelocity runaways from thermonuclear supernovae

Kareem El-Badry, Klaus Werner, Ken J. Shen +16

The explosion of a white dwarf (WD) in a close binary can launch a surviving runaway star at velocities of . Such runaways provide a direct probe of…

astro-ph.SR2026

Chemical Signatures of AGB Mass Transfer in Gaia White Dwarf Companions

Natsuko Yamaguchi, Kareem El-Badry, Henrique Reggiani +2

We present a homogeneous abundance analysis of 160 main-sequence stars in astrometric white-dwarf + main-sequence (WD+MS) binaries with orbits from Gaia DR3. These systems have AU-…

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

Population demographics of white dwarf binaries with intermediate separations: Gaia constraints on post-AGB mass transfer

Natsuko Yamaguchi, Kareem El-Badry, Sahar Shahaf

Astrometry from the Gaia mission has revealed a large population of white dwarf (WD) + main sequence (MS) binaries with periods of d. These systems have separations i…