Phosphorus-related species are not known to be as omnipresent in space as hydrogen,
carbon, nitrogen, oxygen, and sulfur-bearing species. Astronomers spotted very few P …

It is speculated that there might be some linkage between interstellar aldehydes and their
corresponding alcohols. Here an observational study and astrochemical modeling are …

After hydrogen, oxygen, and carbon, nitrogen is one of the most chemically active species in
the interstellar medium. Nitrogen-bearing molecules are very important as they are actively …

It has been pointed out by various astronomers that a very interesting relationship exists
between interstellar alcohols and the corresponding thiols (sulfur analog of alcohols) as far …

Chemical Modeling for Predicting the Abundances of Certain Aldimines and Amines in Hot
Cores - IOPscience This site uses cookies. By continuing to use this site you agree to our use …

Straight-chain (normal-propyl cyanide,) and branched-chain (iso-propyl cyanide,) alkyl
cyanides are recently identified in the massive star-forming regions (Sgr B2 (N) and Orion) …

The molecular species C3H4O represents a striking example of an astrochemical
conundrum. With more than 60 structural isomers theoretically possible, to date only acrolein …

One of the major obstacles to accurately modeling the interstellar chemistry is inadequate
knowledge of the binding energy (BE) of interstellar species with dust grains. In denser …

The abundance of interstellar ice constituents is usually expressed with respect to the water
ice because, in denser regions, a significant portion of the interstellar grain surface would be …

Formation routes, involving closed shell, radical, and charged species for urea, have been
studied using computational methods to probe their feasibility in the interstellar medium. All …