Changjian Xie

activity

20132026

most citedLow temperature rate constants for the N(4S) + CH(X2Πr) reaction. Implications for N2 formation cycles in dense interstellar clouds

37 citations · 155 across the 12 of their papers we have counts for

collaborators

Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2017★ 11 cited

The ortho-to-para ratio of H $_{2}$ Cl $^{+}$ : Quasi-classical trajectory calculations and new simulations in light of new observations

Romane Le Gal, Changjian Xie, Eric Herbst +3

Multi-hydrogenated species with proper symmetry properties can present different spin configurations, and thus exist under different spin symmetry forms, labeled as para and ortho…

astro-ph.GA2016★ 8 cited

The ortho-to-para ratio of interstellar NH $_{2}$ : Quasi-classical trajectory calculations and new simulations

Romane Le Gal, Eric Herbst, Changjian Xie +2

Based on recent $H er sc h e l$ results, the ortho-to-para ratio (OPR) of NH $_{2}$ has been measured towards the following high-mass star-forming regions: W31C (G10.6-0.4), W49N (G43.2-0.…

astro-ph.GA2013★ 37 cited

Low temperature rate constants for the N(4S) + CH(X2Πr) reaction. Implications for N2 formation cycles in dense interstellar clouds

Julien Daranlot, Xixi Hu, Changjian Xie +7

Rate constants for the potentially important interstellar N(4S) + CH(X2Πr) reaction have been measured in a continuous supersonic flow reactor over the range 56 K < T < 296 K using…

The ortho-to-para ratio of H2​Cl+: Quasi-classical trajectory calculations and new simulations in light of new observations

The ortho-to-para ratio of interstellar NH2​: Quasi-classical trajectory calculations and new simulations

Low temperature rate constants for the N(4S) + CH(X2Πr) reaction. Implications for N2 formation cycles in dense interstellar clouds

The ortho-to-para ratio of H $_{2}$ Cl $^{+}$ : Quasi-classical trajectory calculations and new simulations in light of new observations

The ortho-to-para ratio of interstellar NH $_{2}$ : Quasi-classical trajectory calculations and new simulations