Context. Recent observations suggest that planet formation starts early, in protostellar disks
of≤ 10 5 yr, which are characterized by strong interactions with the environment, such as …

Context. In the extremely cold and dark environments of pre-stellar cores, methanol is
formed on the surface of interstellar dust grains and released into the gas phase via non …

Deuterated methanol is one of the most robust windows astrochemists have on the
individual chemical reactions forming deuterium-bearing molecules and the …

Gas phase Elemental abundances in Molecular CloudS (GEMS) is an IRAM 30 m Large
Program designed to provide estimates of the S, C, N, and O depletions and gas ionization …

Stars like our Sun form in self-gravitating dense and cold structures within interstellar clouds
that are referred to as pre-stellar cores. Although much is known about the physical structure …

The internal structure of the prestellar core G208. 68-19.02-N2 (G208-N2) in the Orion
Molecular Cloud 3 (OMC-3) region has been studied with the Atacama Large Millimeter …

Context. In the centre of pre-stellar cores, deuterium fractionation is enhanced due to low
temperatures and high densities. Therefore, the chemistry of deuterated molecules can be …

We present the spectra of complex organic molecules (COMs) detected in HOPS 373SW
with the Atacama Large Millimeter/submillimeter Array (ALMA). HOPS 373SW, which is a …

Context. Deuteration is a crucial tool for understanding the complexity of interstellar
chemical processes, especially when they involve the interplay of gas-phase and grain …

We aim to quantify the effect of chemistry on the infall velocity in the prestellar core L1544.
Previous observational studies have found evidence for double-peaked line profiles for the …