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 …

To date, 204 individual molecular species, comprised of 16 different elements, have been
detected in the interstellar and circumstellar medium by astronomical observations. These …

The evolution of star-forming regions and their thermal balance are strongly influenced by
their chemical composition, which, in turn, is determined by the physicochemical processes …

Recent observational and experimental evidence for the presence of complex organics in
space is reviewed. Remote astronomical observations have detected ∼∼ 200 gas-phased …

To date, 241 individual molecular species, composed of 19 different elements, have been
detected in the interstellar and circumstellar medium by astronomical observations. These …

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

The high abundances of Complex Organic Molecules (COMs) with respect to methanol, the
most abundant COM, detected toward low-mass protostars, tend to be underpredicted by …

Context. Complex organic species are known to be abundant toward low-and high-mass
protostars. No statistical study of these species toward a large sample of high-mass …

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 an unbiased spectral line survey towards the Galactic Centre (GC) quiescent
giant molecular cloud, G+ 0.693 using the GBT and IRAM 30 telescopes. Our study …