https://www.selleckchem.com/products/CX-3543.html
Our results can be further used for modeling fluids in a system of interconnected pores using Monte Carlo and density functional theory methods.Sequential formation of a poly-cyclic aromatic hydrocarbon (PAH) dication in the H I regions of the interstellar medium (ISM) is proposed to be a function of internal energy of the doubly ionized PAHs, which, in turn, is dependent on the single- and double-ionization potentials of the system. This sets a limit on the single- and double-ionization energies of the system(s) that can further underg
Like
Comment
Share
