Observational advances over the last decade have enabled high-resolution, interferometric
studies of forming multiple systems, statistical surveys of multiplicity in star-forming regions …

Stellar multiplicity is a ubiquitous outcome of the star-formation process. The frequency and
main characteristics of multiple systems, and their dependence on primary mass and …

We compile observations of early-type binaries identified via spectroscopy, eclipses, long-
baseline interferometry, adaptive optics, common proper motion, etc. Each observational …

We present the results of the Gould's Belt Distances Survey of young star-forming regions
toward the Orion Molecular Cloud Complex. We detected 36 young stellar objects (YSOs) …

We report the statistical properties of stars, brown dwarfs and multiple systems obtained from
the largest radiation hydrodynamical simulation of star cluster formation to date that resolves …

The supermassive black hole at the center of the Milky Way plays host to a massive, young
cluster that may have formed in one of the most inhospitable environments in the Galaxy. We …

We have conducted a high-resolution imaging study of the Taurus–Auriga star-forming
region in order to characterize the primordial outcome of multiple star formation and the …

We report the statistical properties of stars, brown dwarfs and multiple systems obtained from
the largest hydrodynamical simulation of star cluster formation to date that resolves masses …

We present a multiplicity study of all known protostars (94) in the Perseus molecular cloud
from a Karl G. Jansky Very Large Array survey at Ka-band (8 mm and 1 cm) and C-band (4 …

Context. The lack of high-precision long-term continuous photometric data for large samples
of stars has impeded the large-scale exploration of pulsational variability in the OB star …