SIMBAD references

2017MNRAS.468L...1S - Mon. Not. R. Astron. Soc., 468, L1-L5 (2017/June-2)

New quantum chemical computations of formamide deuteration support gas-phase formation of this prebiotic molecule.

SKOUTERIS D., VAZART F., CECCARELLI C., BALUCANI N., PUZZARINI C. and BARONE V.

Abstract (from CDS):

Based on recent work, formamide might be a potentially very important molecule in the emergence of terrestrial life. Although detected in the interstellar medium for decades, its formation route is still debated, whether in the gas phase or on the dust grain surfaces. Molecular deuteration has proven to be, in other cases, an efficient way to identify how a molecule is synthesized. For formamide, new published observations towards the IRAS16293-2422 B hot corino show that its three deuterated forms have all the same deuteration ratio, 2-5 per cent and that this is a factor of 3-8 smaller than that measured for H2CO towards the IRAS16293-2422 protostar. Following a previous work on the gas-phase formamide formation via the reaction NH2 + H2CO - HCONH2 + H, we present here new calculations of the rate coefficients for the production of monodeuterated formamide through the same reaction, starting from monodeuterated NH2 or H2CO. Some misconceptions regarding our previous treatment of the reaction are also cleared up. The results of the new computations show that, at the 100 K temperature of the hot corino, the rate of deuteration of the three forms is the same, within 20 per cent. On the contrary, the reaction between non-deuterated species proceeds three times faster than that with deuterated ones. These results confirm that a gas-phase route for the formation of formamide is perfectly in agreement with the available observations.

Abstract Copyright:

Journal keyword(s): ISM: abundances - ISM: molecules - ISM: molecules

Simbad objects: 2

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2017MNRAS.468L...1S and select 'bookmark this link' or equivalent in the popup menu


2020.01.26-13:51:39

© Université de Strasbourg/CNRS

    • Contact