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 …

Star-forming regions show a rich and varied chemistry, including the presence of complex
organic molecules—in both the cold gas distributed on large scales and the hot regions …

The interstellar medium is characterized by a rich and diverse chemistry. Many of its
complex organic molecules are proposed to form through radical chemistry in icy grain …

Context. The inner regions of the envelopes surrounding young protostars are characterized
by a complex chemistry, with prebiotic molecules present on the scales where …

Cometary nuclei contain the least modified material from the formative epoch of our
planetary system, and their compositions reflect a range of processes experienced by …

Our Sun and planetary system were born about 4.5 billion years ago. How did this happen,
and what is the nature of our heritage from these early times? This review tries to address …

The cross-disciplinary field of astrochemistry exists to understand the formation, destruction,
and survival of molecules in astrophysical environments. Molecules in space are …

While astrochemical models are successful in reproducing many of the observed interstellar
species, they have been struggling to explain the observed abundances of complex organic …

We present the results of chemical modeling of complex organic molecules (COMs) under
conditions typical for prestellar cores. We utilize an advanced gas-grain astrochemical …

Context. Complex organic molecules (COMs) have long been detected in the interstellar
medium, especially in hot cores and in the hot corinos of low-mass protostars. Their …