The ALMA Survey of Star Formation and Evolution in Massive Protoclusters with Blue Profiles (ASSEMBLE): Core Growth, Cluster Contraction, and Primordial Mass Segregation

• Published in: The Astrophysical journal. Supplement series Vol. 270; no. 1; pp. 9 - 39
• Main Authors: Xu, Fengwei, Wang, Ke, Liu, Tie, Tang, Mengyao, Evans II, Neal J., Palau, Aina, Morii, Kaho, He, Jinhua, Sanhueza, Patricio, Liu, Hong-Li, Stutz, Amelia, Zhang, Qizhou, Chen, Xi, Li, Pak Shing, Gómez, Gilberto C., Vázquez-Semadeni, Enrique, Li, Shanghuo, Mai, Xiaofeng, Lu, Xing, Liu, Meizhu, Chen, Li, Li, Chuanshou, Shi, Hongqiong, Ren, Zhiyuan, Li, Di, Garay, Guido, Bronfman, Leonardo, Dewangan, Lokesh, Juvela, Mika, Lee, Chang Won, Zhang, S., Yue, Nannan, Wang, Chao, Ge, Yifei, Jiao, Wenyu, Luo, Qiuyi, Zhou, J.-W., Tatematsu, Ken’ichi, Chibueze, James O., Su, Keyun, Sun, Shenglan, Ristorcelli, I., Toth, L. Viktor
• Format: Journal Article
• Language: English
• Published: Saskatoon The American Astronomical Society 01.01.2024; IOP Publishing
• Subjects: Accretion; Clumps; Cores; Deposition; Evolution; Infrared signatures; Interstellar medium; Massive stars; Protoclusters; Protostars; Radio telescopes; Star & galaxy formation; Star clusters; Star formation; Star forming regions; Stars; Stellar evolution
• ISSN: 0067-0049; 1538-4365
• DOI: 10.3847/1538-4365/acfee5

Abstract The Atacama Large Millimeter/submillimeter Array (ALMA) Survey of Star Formation and Evolution in Massive Protoclusters with Blue Profiles (ASSEMBLE) aims to investigate the process of mass assembly and its connection to high-mass star formation theories in protoclusters in a dynamic view. We observed 11 massive ( M clump ≳ 10 3 M ⊙ ), luminous ( L bol ≳ 10 4 L ⊙ ), and blue-profile (infall signature) clumps by ALMA with resolution of ∼2200–5500 au (median value of 3500 au) at 350 GHz (870 μ m). We identified 248 dense cores, including 106 cores showing protostellar signatures and 142 prestellar core candidates. Compared to early stage infrared dark clouds (IRDCs) by ASHES, the core mass and surface density within the ASSEMBLE clumps exhibited a significant increment, suggesting concurrent core accretion during the evolution of the clumps. The maximum mass of prestellar cores was found to be 2 times larger than that in IRDCs, indicating that evolved protoclusters have the potential to harbor massive prestellar cores. The mass relation between clumps and their most massive core (MMCs) is observed in ASSEMBLE but not in IRDCs, which is suggested to be regulated by multiscale mass accretion. The mass correlation between the core clusters and their MMCs has a steeper slope compared to that observed in stellar clusters, which can be due to fragmentation of the MMC and stellar multiplicity. We observe a decrease in core separation and an increase in central concentration as protoclusters evolve. We confirm primordial mass segregation in the ASSEMBLE protoclusters, possibly resulting from gravitational concentration and/or gas accretion.