Hu, Y., & Yang, J. (2014). Role of ocean heat transport in climates of tidally locked exoplanets around M dwarf stars. Proceedings of the National Academy of Sciences - PNAS, 111(2), 629. https://doi.org/10.1073/pnas.1315215111
Citácia podle Chicago (17th ed.)Hu, Yongyun, a Jun Yang. "Role of Ocean Heat Transport in Climates of Tidally Locked Exoplanets Around M Dwarf Stars." Proceedings of the National Academy of Sciences - PNAS 111, no. 2 (2014): 629. https://doi.org/10.1073/pnas.1315215111.
Citácia podľa MLA (8th ed.)Hu, Yongyun, a Jun Yang. "Role of Ocean Heat Transport in Climates of Tidally Locked Exoplanets Around M Dwarf Stars." Proceedings of the National Academy of Sciences - PNAS, vol. 111, no. 2, 2014, p. 629, https://doi.org/10.1073/pnas.1315215111.
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