Cite
Is the gas-phase OH+H 2 CO reaction a source of HCO in interstellar cold dark clouds? A kinetic, dynamic and modelling study.
MLA
Ocaña, A. J., et al. “Is the Gas-Phase OH+H 2 CO Reaction a Source of HCO in Interstellar Cold Dark Clouds? A Kinetic, Dynamic and Modelling Study.” The Astrophysical Journal, vol. 850, no. 1, Nov. 2017. EBSCOhost, https://doi.org/10.3847/1538-4357/aa93d9.
APA
Ocaña, A. J., Jiménez, E., Ballesteros, B., Canosa, A., Antiñolo, M., Albaladejo, J., Agúndez, M., Cernicharo, J., Zanchet, A., Del Mazo, P., Roncero, O., & Aguado, A. (2017). Is the gas-phase OH+H 2 CO reaction a source of HCO in interstellar cold dark clouds? A kinetic, dynamic and modelling study. The Astrophysical Journal, 850(1). https://doi.org/10.3847/1538-4357/aa93d9
Chicago
Ocaña, A J, E Jiménez, B Ballesteros, A Canosa, M Antiñolo, J Albaladejo, M Agúndez, et al. 2017. “Is the Gas-Phase OH+H 2 CO Reaction a Source of HCO in Interstellar Cold Dark Clouds? A Kinetic, Dynamic and Modelling Study.” The Astrophysical Journal 850 (1). doi:10.3847/1538-4357/aa93d9.