Research

The majority of stars have companions, making binary and triple star systems a fundamental part of stellar evolution. My work focuses on understanding the physical processes that shape the evolution of multiple star systems and their population-wide properties. See Publications for a full list of papers.

Triple Stars

Triples are common and dynamically rich, offering a natural laboratory for studying stellar mergers, population evolution, and the origins of exotic stellar phenomena. Much of my work on triples is carried out in collaboration with Smadar Naoz, focusing on how 3-body dynamics couple to stellar evolution and mass transfer.

Pan-STARRS image of a resolved triple from Gaia, with proper-motion arrows Pan-STARRS image of a resolved triple white dwarf from Gaia, with proper-motion arrows
Two resolved triples from Gaia. Blue arrows mark the proper motions of the three stars in each triple; red arrows mark unrelated field stars. From Shariat, El-Badry & Naoz (2025).

Binary Stars

Binaries are ubiquitous and form the inner building blocks of triples and higher-order systems. I’m interested in understanding the physical processes that govern binary evolution, such as constraining the outcomes of binary mass transfer, through observations and theoretical modeling.

ZTF light curves of three eclipsing white dwarf-main sequence binaries
ZTF light curves of eclipsing white dwarf–main sequence binaries that survived a phase of unstable mass transfer (common-envelope evolution), phase-folded on their orbital periods. From Shariat & El-Badry (2026).

I also study binary populations in other galaxies, from ultra-faint dwarfs to the Whirlpool Galaxy.

Hubble image of the Whirlpool Galaxy with the survey footprints, and the light curve of one eclipsing binary
The Whirlpool Galaxy (M51) imaged by Hubble, with the ACS (cyan) and WFC3 (yellow) footprints used to find 173 massive eclipsing-binary candidates. The inset shows the light curve of one of them (white box), folded on its 2.32-day orbital period. From Shariat et al. (2026).

Broader Interests

Alongside these core themes, I remain curious about related problems across astrophysics, many of which still involve binaries. I have used wide binaries to calibrate the precision of stellar ages and Gaia to test whether long secondary periods in red giants have a binary origin. I am also interested in planets, including how stellar companions shape hot Jupiters and how multi-planet systems form.

Cartoon of a hot Jupiter on a misaligned orbit around its star, with a distant stellar companion Bar chart: hot Jupiters with a detected stellar companion are about twice as often misaligned
Hot Jupiters with a distant stellar companion are twice as likely to be misaligned. From Shariat et al. (2026).