Cosmic evolution of molecular gas mass density from an empirical relationship between L1.4 GHz and L′CO.

MLA

Orellana-González, G., et al. “Cosmic Evolution of Molecular Gas Mass Density from an Empirical Relationship between L1.4 GHz and L′CO.” Monthly Notices of the Royal Astronomical Society, vol. 495, no. 2, June 2020, pp. 1760–70. EBSCOhost, https://doi.org/10.1093/mnras/staa1171.

APA

Orellana-González, G., Ibar, E., Leiton, R., Thomson, A. P., Cheng, C., Ivison, R. J., Herrera-Camus, R., Messias, H., Calderón-Castillo, P., Hughes, T. M., & Leeuw, L. (2020). Cosmic evolution of molecular gas mass density from an empirical relationship between L1.4 GHz and L′CO. Monthly Notices of the Royal Astronomical Society, 495(2), 1760–1770. https://doi.org/10.1093/mnras/staa1171

Chicago

Orellana-González, G, E Ibar, R Leiton, A P Thomson, C Cheng, R J Ivison, R Herrera-Camus, et al. 2020. “Cosmic Evolution of Molecular Gas Mass Density from an Empirical Relationship between L1.4 GHz and L′CO.” Monthly Notices of the Royal Astronomical Society 495 (2): 1760–70. doi:10.1093/mnras/staa1171.