Hydroxylamine, NH2OH, is one of the already detected interstellar molecules with the highest prebiotic potential. Yet, the abundance of this molecule found by astronomical observations is rather low for a […]
Interstellar
Searching For Life With Space Dust
Following enormous collisions, such as asteroid impacts, some amount of material from an impacted world may be ejected into space.
The Chemistry Of H2NC In The Interstellar Medium And The Role Of The C + NH3 Reaction
We carried out an observational search for the recently discovered molecule H2NC, and its more stable isomer H2CN, toward eight cold dense clouds (L1544, L134N, TMC-2, Lupus-1A, L1489, TMC-1 NH3, […]
Are We Alone? University Engages Satellite Company In A Search For Life Among The Stars
The University of Sydney has signed a contract with EnduroSat, a leading provider of micro satellites and space services, to explore the question of life beyond Earth, starting with our […]
ALMA Traces The History Of Water In Planet Formation Back To The Interstellar Medium
Scientists studying a nearby protostar have detected the presence of water in its circumstellar disk. The new observations made with the Atacama Large Millimeter/submillimeter Array (ALMA) mark the first detection […]
Could Nucleobases Form In The ISM? A Theoretical Study In The Horsehead Nebula
This work presents the results of a theoretical study that analyzed the possibility of nucleobases to form in the interstellar medium, in the Horsehead nebula, which is a region considered […]
Chemical Models Of Adenine Precursors Cyanamide And Carbodiimide In The Interstellar Medium
Cyanamide (NH2CN) and its isomer, carbodiimide (HNCNH), may form adenine in the interstellar medium (ISM) via a series of reactions.
Interstellar Complex Organic Molecules Towards Outflows From The G351.16+0.70 (NGC 6334 V) Massive Protostellar System
G351.16+0.70 is a relatively well-studied High Mass Star Forming Region with at least two main bipolar outflow structures originating from an OB embedded star and multiple IR cores.
Radio Recombination Lines Of Carbon/Oxygen Ions Detected For The First Time
A research team from the Shanghai Astronomical Observatory (SHAO) of the Chinese Academy of Sciences has detected radio recombination lines (RRLs) of ions heavier than helium for the first time, […]
Resonant Infrared Irradiation Of CO And CH3OH Interstellar Ices
Solid-phase photo-processes involving icy dust grains greatly affect the chemical evolution of the interstellar medium by leading to the formation of complex organic molecules and by inducing photodesorption.
