Cite
Non-LTE line formation of Fe in late-type stars - I. Standard stars with 1D and 〈3D〉 model atmospheres.
MLA
Bergemann, Maria, et al. “Non-LTE Line Formation of Fe in Late-Type Stars - I. Standard Stars with 1D and 〈3D〉 Model Atmospheres.” Monthly Notices of the Royal Astronomical Society, vol. 427, no. 1, Nov. 2012, pp. 27–49. EBSCOhost, https://doi.org/10.1111/j.1365-2966.2012.21687.x.
APA
Bergemann, M., Lind, K., Collet, R., Magic, Z., & Asplund, M. (2012). Non-LTE line formation of Fe in late-type stars - I. Standard stars with 1D and 〈3D〉 model atmospheres. Monthly Notices of the Royal Astronomical Society, 427(1), 27–49. https://doi.org/10.1111/j.1365-2966.2012.21687.x
Chicago
Bergemann, Maria, K. Lind, R. Collet, Z. Magic, and M. Asplund. 2012. “Non-LTE Line Formation of Fe in Late-Type Stars - I. Standard Stars with 1D and 〈3D〉 Model Atmospheres.” Monthly Notices of the Royal Astronomical Society 427 (1): 27–49. doi:10.1111/j.1365-2966.2012.21687.x.