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 …

This review is concerned with the formation of molecules in the interstellar medium (ISM),
which is composed mainly of regions of gas and dust known as interstellar clouds, ranging …

A new, more comprehensive model of gas–grain chemistry in hot molecular cores is
presented, in which nondiffusive reaction processes on dust-grain surfaces and in ice …

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

Based on sub-arcsecond Atacama Large Millimeter/submillimeter Array (ALMA) and
Submillimeter Array (SMA) 1.3 mm continuum images of the massive protocluster NGC …

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 formation of the interstellar complex organic molecules (iCOMs) is a hot topic in
astrochemistry. One of the main paradigms trying to reproduce the observations postulates …

To understand how phosphorus (P)-bearing molecules are formed in star-forming regions,
we have analysed the Atacama Large Millimeter/Submillimeter Array (ALMA) observations …

Interstellar formamide (NH2CHO) has recently attracted significant attention due to its
potential role as a molecular building block in the formation of precursor biomolecules …

Ethanol (CH3CH2OH) is a relatively common molecule, often found in star-forming regions.
Recent studies suggest that it could be a parent molecule of several so-called interstellar …