Pathways for the Formation of Formamide, a Prebiotic Biomonomer: Metal-Ions in Interstellar Gas-Phase Chemistry

2021 ◽  
Vol 125 (16) ◽  
pp. 3457-3472
Author(s):  
Sorakayala Thripati ◽  
Raghunath O. Ramabhadran
1993 ◽  
Vol 89 (13) ◽  
pp. 2193 ◽  
Author(s):  
Bertrand R. Rowe ◽  
Andr� Canosa ◽  
Ian R. Sims

1983 ◽  
Vol 16 (3) ◽  
pp. 215-219 ◽  
Author(s):  
S. K. Huang ◽  
Y. C. Lee ◽  
J. Allison ◽  
A. I. Popov

1989 ◽  
Vol 8 ◽  
pp. 383-386
Author(s):  
David A. Williams

ABSTRACTThe chemical effects of interstellar grains are briefly reviewed. Their dominant chemical role is to catalyze the formation of H2 which is the seminal molecule for efficient gas phase chemistry. In regions of at least moderate extinction grains accumulate molecular mantles of CO, H2O, etc. Solid state chemistry in such mantles may produce molecules of a type or in an abundance not achievable in the interstellar gas. Return of mantle material to the gas can – at least transiently – dominate gas phase chemistry. It is argued that the freeze-out of heavy atomic and molecular species on to grain surfaces limits the time available for chemistry, restricts molecular cloud chemistry to a “young” character, and suggests that chemical models of molecular clouds must have cyclic dynamics. Such models are briefly described.


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