The disks that orbit young stars are the essential conduits and reservoirs of material for star
and planet formation. Their structures, meaning the spatial variations of the disk physical …

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

Context. In the past few years, there has been a rise in the detection of streamers,
asymmetric flows of material directed toward the protostellar disk with material from outside …

We solve the equations of two-dimensional hydrodynamics describing a circumbinary disk
accreting onto an eccentric, equal-mass binary. We compute the time rate of change of the …

Using high-resolution hydrodynamics simulations, we show that equal-mass binaries
accreting from a circumbinary disk evolve toward an orbital eccentricity of e≃ 0.45, unless …

We report spectro-polarimetric results of an observational campaign of the bright neutron
star low-mass X-ray binary Cyg X-2 simultaneously observed by IXPE, NICER, and …

Context. The infall of gas from outside natal cores has proven to feed protostars after the
main accretion phase (Class 0). This changes our view of star formation to a picture that …

Stars collect most of their mass during the protostellar stage, yet the accretion luminosity and
stellar parameters, which are needed to compute the mass accretion rate, are poorly …

Modern numerical hydrodynamics tools have recently enabled detailed examinations of
binaries accreting from prograde circumbinary discs. These have reframed the current …

We characterize protostellar multiplicity in the Orion molecular clouds using Atacama Large
Millimeter/submillimeter Array 0.87 mm and Very Large Array 9 mm continuum surveys …