Cite
ALMA CO observations of a giant molecular cloud in M 33: Evidence for high-mass star formation triggered by cloud–cloud collisions.
MLA
Sano, Hidetoshi, et al. “ALMA CO Observations of a Giant Molecular Cloud in M 33: Evidence for High-Mass Star Formation Triggered by Cloud–cloud Collisions.” Publications of the Astronomical Society of Japan, vol. 73, Jan. 2021, pp. 1–13. EBSCOhost, https://doi.org/10.1093/pasj/psaa045.
APA
Sano, H., Tsuge, K., Tokuda, K., Muraoka, K., Tachihara, K., Yamane, Y., Kohno, M., Fujita, S., Enokiya, R., Rowell, G., Maxted, N., Filipović, M. D., Knies, J., Sasaki, M., Onishi, T., Plucinsky, P. P., & Fukui, Y. (2021). ALMA CO observations of a giant molecular cloud in M 33: Evidence for high-mass star formation triggered by cloud–cloud collisions. Publications of the Astronomical Society of Japan, 73, 1–13. https://doi.org/10.1093/pasj/psaa045
Chicago
Sano, Hidetoshi, Kisetsu Tsuge, Kazuki Tokuda, Kazuyuki Muraoka, Kengo Tachihara, Yumiko Yamane, Mikito Kohno, et al. 2021. “ALMA CO Observations of a Giant Molecular Cloud in M 33: Evidence for High-Mass Star Formation Triggered by Cloud–cloud Collisions.” Publications of the Astronomical Society of Japan 73 (January): 1–13. doi:10.1093/pasj/psaa045.