Cite
Filamentary mass accretion towards the high-mass protobinary system G11.92–0.61 MM2.
MLA
张遂楠), S Zhang, et al. “Filamentary Mass Accretion towards the High-Mass Protobinary System G11.92–0.61 MM2.” Monthly Notices of the Royal Astronomical Society, vol. 533, no. 1, Sept. 2024, pp. 1075–94. EBSCOhost, https://doi.org/10.1093/mnras/stae1844.
APA
张遂楠), S Zhang, Cyganowski, C. J., Henshaw, J. D., Brogan, C. L., Hunter, T. R., Friesen, R. K., Bonnell, I. A., & Viti, S. (2024). Filamentary mass accretion towards the high-mass protobinary system G11.92–0.61 MM2. Monthly Notices of the Royal Astronomical Society, 533(1), 1075–1094. https://doi.org/10.1093/mnras/stae1844
Chicago
张遂楠), S Zhang, C J Cyganowski, J D Henshaw, C L Brogan, T R Hunter, R K Friesen, I A Bonnell, and S Viti. 2024. “Filamentary Mass Accretion towards the High-Mass Protobinary System G11.92–0.61 MM2.” Monthly Notices of the Royal Astronomical Society 533 (1): 1075–94. doi:10.1093/mnras/stae1844.