المؤلفون: 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

المساهمون: Department of Physics

مصطلحات موضوعية: Infrared dark cloud, Compact source catalog, Scale greater-than-or-equal-to-10 pc, Radiation-hydrodynamic simulations, Velocity-coherent filaments, Thermal jeans fragmentation, Large array observations, Inner galactic plane, Forming regions, Hierarchical fragmentation, Astronomy, Space science

وصف الملف: application/pdf

Relation: We thank the anonymous referee for the constructive comments. This work has been supported by the National Science Foundation of China (11973013, 12033005, 11721303, 12073061, 12122307, 12203011, 12103045) and the National Key R&D Program of China (Nos. 2022YFA1603100, 2019YFA0405100). F.W.X. and K.W. acknowledge support from the China Manned Space Project (CMS-CSST-2021-A09, CMS-CSST-2021-B06), the High-Performance Computing Platform of Peking University, and the China-Chile Joint Research Fund (CCJRF No. 2211). CCJRF is provided by the Chinese Academy of Sciences South America Center for Astronomy (CASSACA) and established by the National Astronomical Observatories, Chinese Academy of Sciences (NAOC) and the Chilean Astronomy Society (SOCHIAS) to support Chinese-Chilean collaborations in astronomy. T.L. acknowledges the support by the international partnership program of Chinese academy of sciences through grant No. 114231KYSB20200009, and Shanghai Pujiang Program 20PJ1415500. M.Y.T. acknowledges the support by Yunnan provincial Department of Science and Technology through grant No. 202101BA070001-261. K.M. is financially supported by Grants-in-Aid for the Japan Society for the Promotion of Science (JSPS) Fellows (KAKENHI No. 22J21529). P.S. was partially supported by a Grant-in-Aid for Scientific Research (KAKENHI Nos. JP22H01271 and JP23H01221) of JSPS. H.L.L. is supported by Yunnan Fundamental Research Project (grant No. 202301AT070118). A.P., G.C.G., and E.V.S. acknowledge financial support from the UNAM-PAPIIT IG100223 grant. A.P. acknowledges financial support from the Sistema Nacional de Investigadores of CONAHCyT, and from the CONAHCyT project No. 86372 of the "Ciencia de Frontera 2019" program, entitled "Citlalcoatl: A multiscale study at the new frontier of the formation and early evolution of stars and planetary systems," Mexico. G.C.G. acknowledges support from UNAM-PAPIIT IN10382 grant. A.S., G.G., and L.B. gratefully acknowledge support of ANID through the BASAL project FB210003. A.S. also gratefully acknowledges support from the Fondecyt Regular (project code 1220610). This work is sponsored (in part) by the Chinese Academy of Sciences (CAS), through a grant to the CAS South America Center for Astronomy (CASSACA) in Santiago, Chile. M.J. acknowledges the support of the Academy of Finland grant No. 348342. C.W.L. is supported by the Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education, Science and Technology (NRF- 2019R1A2C1010851), and by the Korea Astronomy and Space Science Institute grant funded by the Korea government (MSIT; project No. 2023-1-84000). K.T. was supported by JSPS KAKENHI (grant No. JP20H05645). This paper uses the following ALMA data: ADS/JAO.ALMA#2017.1.00545.S and 2019.1.00685.S, and ADS/JAO.ALMA#2015.1.01539.S, 2017.1.00716.S, and 2018.1.00192.S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada), Molonglo Observatory Synthesis Telescope (MOST) and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. Data analysis was in part carried out on the High-Performance Computing Platform of Peking University, and the open-use data analysis computer system at the Astronomy Data Center (ADC) of the National Astronomical Observatory of Japan. r The MeerKAT telescope is operated by the South African Radio Astronomy Observatory, which is a facility of the National Research Foundation, an agency of the Department of Science and Innovation.; Xu , F , Wang , K , Liu , T , Tang , M , Evans II , N J , Palau , A , Morii , K , He , J , Sanhueza , P , Liu , H-L , Stutz , A , Zhang , Q , Chen , X , Li , P S , Gómez , G C , Vázquez-Semadeni , E , Li , S , Mai , X , Lu , X , Liu , M , Chen , L , Li , C , Shi , H , Ren , Z , Li , D , Garay , G , Bronfman , L , Dewangan , L , Juvela , M , Lee , C W , Zhang , S , Yue , N , Wang , C , Ge , Y , Jiao , W , Luo , Q , Zhou , J-W , Tatematsu , K , Chibueze , J O , Su , K , Sun , S , Ristorcelli , I & Toth , L V 2024 , ' The ALMA Survey of Star Formation and Evolution in Massive Protoclusters with Blue Profiles (ASSEMBLE) : Core Growth, Cluster Contraction, and Primordial Mass Segregation ' , Astrophysical Journal Supplement Series , vol. 270 , no. 1 , 9 . https://doi.org/10.3847/1538-4365/acfee5; ORCID: /0000-0002-5809-4834/work/156653361; http://hdl.handle.net/10138/573648; 467bddc5-10d6-4073-8280-700763a51bf0; 001132952700001

الاتاحة: http://hdl.handle.net/10138/573648

المؤلفون: Xu, Fengwei, Wang, Ke, Liu, Tie, Tang, Mengyao, Evans, Neal J., II, Palau, Aina, Morii, Kaho, He, Jinhua, Sanhueza, Patricio, Liu, Hong-Li, Stutz, Amelia, Zhang, Qizhou, Chen, Xi, Li, Pak Shing, Gomez, Gilberto C., Vazquez-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

مصطلحات موضوعية: Astronomy & Astrophysics, INFRARED DARK CLOUD, COMPACT SOURCE CATALOG, SCALE GREATER-THAN-OR-EQUAL-TO-10 PC, RADIATION-HYDRODYNAMIC SIMULATIONS, VELOCITY-COHERENT FILAMENTS, THERMAL JEANS FRAGMENTATION, LARGE ARRAY OBSERVATIONS, INNER GALACTIC PLANE, FORMING REGIONS, HIERARCHICAL FRAGMENTATION

Relation: ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES; http://ir.ynao.ac.cn/handle/114a53/26661

الاتاحة: http://ir.ynao.ac.cn/handle/114a53/26661
https://doi.org/10.3847/1538-4365/acfee5

المؤلفون: Xu, Fengwei, Wang, Ke, Liu, Tie, Tang, Mengyao, II, Neal J. Evans, Palau, Aina, Morii, Kaho, 何金华, 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

مصطلحات موضوعية: 天文学, 理学, 理学::天文学, Astronomy & Astrophysics, INFRARED DARK CLOUD, COMPACT SOURCE CATALOG, SCALE GREATER-THAN-OR-EQUAL-TO-10 PC, RADIATION-HYDRODYNAMIC SIMULATIONS, VELOCITY-COHERENT FILAMENTS, THERMAL JEANS FRAGMENTATION, LARGE ARRAY OBSERVATIONS, INNER GALACTIC PLANE, FORMING REGIONS, HIERARCHICAL FRAGMENTATION

Relation: ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES; http://ir.ynao.ac.cn/handle/114a53/26479; https://dx.doi.org/10.3847/1538-4365/acfee5

الاتاحة: http://ir.ynao.ac.cn/handle/114a53/26479
https://doi.org/10.3847/1538-4365/acfee5