Cite
The post-common-envelope binary nucleus of the planetary nebula IC~4776: Neither an anomalously long orbital period nor a Wolf-Rayet binary
MLA
Miszalski, B., et al. The Post-Common-Envelope Binary Nucleus of the Planetary Nebula IC~4776: Neither an Anomalously Long Orbital Period nor a Wolf-Rayet Binary. 2019. EBSCOhost, https://doi.org/10.1093/mnras/stz1315.
APA
Miszalski, B., Manick, R., Van Winckel, H., & Mikołajewska, J. (2019). The post-common-envelope binary nucleus of the planetary nebula IC~4776: Neither an anomalously long orbital period nor a Wolf-Rayet binary. https://doi.org/10.1093/mnras/stz1315
Chicago
Miszalski, B., R. Manick, H. Van Winckel, and J. Mikołajewska. 2019. “The Post-Common-Envelope Binary Nucleus of the Planetary Nebula IC~4776: Neither an Anomalously Long Orbital Period nor a Wolf-Rayet Binary.” doi:10.1093/mnras/stz1315.