1.
Chem Commun (Camb)
; 52(42): 6873-6, 2016 May 25.
Article
in English
| MEDLINE
| ID: mdl-27103407
ABSTRACT
Using periodic DFT-D2 methods, atomistic simulations of interstellar H adsorption and H2 formation on a (010) Fe-containing olivine surface are presented. At variance with the (010) Mg2SiO4 surface and key to these processes are the large Fe/H interaction energies, suggesting that olivine surfaces are good reservoirs of H atoms for subsequent recombination to form H2.
2.
Am J Hematol
; 62(1): 63-4, 1999 Sep.
Article
in English
| MEDLINE
| ID: mdl-10467282