The CO(3–2)/CO(1–0) Luminosity Line Ratio in Nearby Star-forming Galaxies and Active Galactic Nuclei from xCOLD GASS, BASS, and SLUGS.

MLA

Isabella Lamperti, et al. “The CO(3–2)/CO(1–0) Luminosity Line Ratio in Nearby Star-Forming Galaxies and Active Galactic Nuclei from XCOLD GASS, BASS, and SLUGS.” Astrophysical Journal, vol. 889, no. 2, Feb. 2020, p. 1. EBSCOhost, https://doi.org/10.3847/1538-4357/ab6221.

APA

Isabella Lamperti, Amélie Saintonge, Michael Koss, Serena Viti, Christine D. Wilson, Hao He, T. Taro Shimizu, Thomas R. Greve, Richard Mushotzky, Ezequiel Treister, Carsten Kramer, David Sanders, Kevin Schawinski, & Linda J. Tacconi. (2020). The CO(3–2)/CO(1–0) Luminosity Line Ratio in Nearby Star-forming Galaxies and Active Galactic Nuclei from xCOLD GASS, BASS, and SLUGS. Astrophysical Journal, 889(2), 1. https://doi.org/10.3847/1538-4357/ab6221

Chicago

Isabella Lamperti, Amélie Saintonge, Michael Koss, Serena Viti, Christine D. Wilson, Hao He, T. Taro Shimizu, et al. 2020. “The CO(3–2)/CO(1–0) Luminosity Line Ratio in Nearby Star-Forming Galaxies and Active Galactic Nuclei from XCOLD GASS, BASS, and SLUGS.” Astrophysical Journal 889 (2): 1. doi:10.3847/1538-4357/ab6221.