Figure 3 from Formation of Interstellar Complex Polycyclic Aromatic Hydrocarbons: Insights from Molecular Dynamics Simulations of Dehydrogenated Benzene

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Formation of Interstellar Complex Polycyclic Aromatic Hydrocarbons: Insights from Molecular Dynamics Simulations of Dehydrogenated Benzene

Authors: Meriem Hanine, Zhisen Meng, Shiru Lu, Peng Xie, Sylvain Picaud, Michel Devel, and Zhao Wang

2020 The Astrophysical Journal 900 188.

Provider: AAS Journals

Caption: Figure 3.

Probability distribution of PAH molecules formed from C₆H (left panels) or C₆H₂ (right panels) at (a), (b) 10; (c), (d) 300; (e), (f) 800 K. The probability is calculated to be the ratio between the number of atoms in the formed molecule over the total number of atoms in the simulation cell.

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