Planets form and obtain their compositions in disks of gas and dust around young stars. The
chemical compositions of these planet-forming disks regulate all aspects of planetary …

Planets form in disks of gas and dust around young stars. The disk molecular reservoirs and
their chemical evolution affect all aspects of planet formation, from the coagulation of dust …

Planets form and obtain their compositions in dust-and gas-rich disks around young stars,
and the outcome of this process is intimately linked to the disk chemical properties. The …

Molecular line observations are powerful tracers of the physical and chemical conditions
across the different evolutionary stages of star, disk, and planet formation. The high angular …

Quantifying the composition of the material in protoplanetary disks is essential to
determining the potential for exoplanetary systems to produce and support habitable …

The chemical composition of gas and ice in disks around young stars sets the bulk
composition of planets. In contrast to protoplanetary disks (Class II), young disks that are still …

The complex organic molecules (COMs) detected in star-forming regions are the precursors
of the prebiotic molecules that can lead to the emergence of life. By studying COMs in more …

Sulfur-bearing molecules play an important role in prebiotic chemistry and planet
habitability. They are also proposed probes of chemical ages, elemental C/O ratio, and grain …

The precursors to larger, biologically relevant molecules are detected throughout interstellar
space, but determining the presence and properties of these molecules during planet …

Aims. We present high-sensitivity and high spectral-resolution NOEMA observations of the
Class 0/I binary system SVS13A, composed of the low-mass protostars VLA4A and VLA4B …