Speaker
Sagar Malhotra
(IEEC-ICCUB)
Description
Precise Gaia astrometry and photometry have enabled large-scale studies of unresolved binaries across the Milky Way. However, most existing (spectro-)photometric techniques based solely on these data remain primarily sensitive to high mass-ratio systems (q ≳ 0.6). In a recent pathfinder study we demonstrated that incorporating near- and mid-infrared photometry—such as from 2MASS and WISE—significantly enhances the detectability of low-q binaries. The exquisite deep all-sky photometry from GaiaNIR will therefore be transformative, enabling a much more complete census of binary populations in the Galaxy and offering new constraints on the processes governing star formation and dynamical interactions.
Author
Sagar Malhotra
(IEEC-ICCUB)
Co-authors
Alfred Castro-Ginard
(Universitat de Barcelona)
Friedrich Anders
(Universitat de Barcelona)