ALMA CO Observations of the Mixed-Morphology Supernova Remnant W49B: Efficient Production of Recombining Plasma and Hadronic Gamma-rays via Shock-Cloud Interactions

MLA

Sano, H., et al. ALMA CO Observations of the Mixed-Morphology Supernova Remnant W49B: Efficient Production of Recombining Plasma and Hadronic Gamma-Rays via Shock-Cloud Interactions. 2021. EBSCOhost, https://doi.org/10.3847/1538-4357/ac0dba.

APA

Sano, H., Yoshiike, S., Yamane, Y., Hayashi, K., Enokiya, R., Tokuda, K., Tachihara, K., Rowell, G., Filipović, M. D., & Fukui, Y. (2021). ALMA CO Observations of the Mixed-Morphology Supernova Remnant W49B: Efficient Production of Recombining Plasma and Hadronic Gamma-rays via Shock-Cloud Interactions. https://doi.org/10.3847/1538-4357/ac0dba

Chicago

Sano, H., S. Yoshiike, Y. Yamane, K. Hayashi, R. Enokiya, K. Tokuda, K. Tachihara, G. Rowell, M. D. Filipović, and Y. Fukui. 2021. “ALMA CO Observations of the Mixed-Morphology Supernova Remnant W49B: Efficient Production of Recombining Plasma and Hadronic Gamma-Rays via Shock-Cloud Interactions.” doi:10.3847/1538-4357/ac0dba.