Where did the Earth’s water come from? Although comets, with their icy nuclei, seem like ideal candidates, analyses have so far shown that their water differs from that in our […]
astrochemistry
Deuterated Forms of H+3 and Their Importance in Astrochemistry
At the low temperatures (∼10 K) and high densities (∼100,000 H2 molecules per cc) of molecular cloud cores and protostellar envelopes, a large amount of molecular species (in particular those […]
Synthesis Of Complex Organic Molecules in Soft x-ray Irradiated Ices
We study the chemical evolution of H2O:CO:NH3 ice mixtures irradiated with soft X-rays, in the range 250-1250 eV. We identify many nitrogen-bearing molecules such as e.g., OCN-, NH4+ , HNCO, […]
Vacuum Ultraviolet Photodesorption and Photofragmentation of Formaldehyde-containing Ices
Non-thermal desorption from icy grains containing H2CO has been invoked to explain the observed H2CO gas phase abundances in ProtoPlanetary Disks (PPDs) and Photon Dominated Regions (PDRs). Photodesorption is thought […]
Extension of the HCOOH and CO2 Solid-state Reaction Network During The CO Freeze-out Stage: Inclusion of H2CO
Formic acid (HCOOH) and carbon dioxide (CO2) are simple species that have been detected in the interstellar medium. The solid-state formation pathways of these species under experimental conditions relevant to […]
Solid-state Formation In A H3CCCH + OH Cocktail Under Dark Cloud Conditions
A number of recent experimental studies have shown that solid-state complex organic molecules (COMs) can form under conditions that are relevant to the CO freeze-out stage in dense clouds. In […]
The Role of N2 as a Geo-Biosignature for the Detection and Characterization of Earth-like Habitats
Since the Archean, N2 has been a major atmospheric constituent in Earth’s atmosphere. Nitrogen is an essential element in the building blocks of life, therefore the geobiological nitrogen cycle is […]
Observations Of CH3OH And CH3CHO In A Sample of Protostellar Outflow Sources
Iram 30-m Observations towards eight protostellar outflow sources were taken in the 96-176 GHz range. Transitions of CH3OH and CH3CHO were detected in seven of them. The integrated emission of […]
Isocyanogen Formation In The Cold Interstellar Medium
Cyanogen (NCCN) is the simplest member of the dicyanopolyynes group, and has been proposed as a major source of the CN radical observed in cometary atmospheres. Although not detected through […]
Dispersion Forces Stabilise Ice Coatings at Certain Gas Hydrate Interfaces Which Prevent Water Wetting
Gas hydrates formed in oceans and permafrost occur in vast quantities on Earth representing both a massive potential fuel source and a large threat in climate forecasts. They have been […]
