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 …

Context. One of the important questions of astrochemistry is how complex organic
molecules, including potential prebiotic species, are formed in the envelopes around …

Context. Complex organic molecules (COMs) have been detected in a few Class 0
protostars but their origin is not well understood. While the usual picture of a hot corino …

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 …

Despite the harsh conditions of the interstellar medium, chemistry thrives in it, especially in
star-forming regions where several interstellar complex organic molecules (iCOMs) have …

The carbon (3 P) atom is a reactive species that, according to laboratory experiments and
theoretical calculations, condensates with interstellar ice components. This fact is of …

Organic molecules are widely present in the dense interstellar medium, and many have
been synthesized in the laboratory on Earth under the conditions typical for an interstellar …

Context. Complex organic molecules (COMs) are thought to form on icy dust grains in the
earliest phase of star formation. The evolution of these COMs from the youngest Class 0/I …

We present the first census of the interstellar Complex Organic Molecules (iCOMs) in the low-
mass Class I protostar SVS13-A, obtained by analysing data from the IRAM-30 m Large …