Xu, X., Chen, X., & Yang, Y. (2025). Cooling process of the high-mass young stellar object G24.33+0.14 following an accretion burst.
Chicago Style (17th ed.) CitationXu, Xiaoyun, Xi Chen, and Yang Yang. Cooling Process of the High-mass Young Stellar Object G24.33+0.14 Following an Accretion Burst. 2025.
MLA (9th ed.) CitationXu, Xiaoyun, et al. Cooling Process of the High-mass Young Stellar Object G24.33+0.14 Following an Accretion Burst. 2025.
Warning: These citations may not always be 100% accurate.