Bell, T. J., & Cowan, N. B. (2018). Increased Heat Transport in Ultra-hot Jupiter Atmospheres through H2 Dissociation and Recombination. Astrophysical journal. Letters, 857(2), . https://doi.org/10.3847/2041-8213/aabcc8
Citace podle Chicago (17th ed.)Bell, Taylor J., a Nicolas B. Cowan. "Increased Heat Transport in Ultra-hot Jupiter Atmospheres Through H2 Dissociation and Recombination." Astrophysical Journal. Letters 857, no. 2 (2018). https://doi.org/10.3847/2041-8213/aabcc8.
Citace podle MLA (9th ed.)Bell, Taylor J., a Nicolas B. Cowan. "Increased Heat Transport in Ultra-hot Jupiter Atmospheres Through H2 Dissociation and Recombination." Astrophysical Journal. Letters, vol. 857, no. 2, 2018, https://doi.org/10.3847/2041-8213/aabcc8.
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