المؤلفون: Peng, Yaping, Liu, Tie, Qin, Sheng-Li, Baug, Tapas, Liu, Hong-Li, Wang, Ke, Garay, Guido, Zhang, Chao, Chen, Long-Fei, Lee, Chang Won, Juvela, Mika, Li, Dalei, Tatematsu, Ken'ichi, Liu, Xun-Chuan, Lee, Jeong-Eun, Luo, Gan, Dewangan, Lokesh, Wu, Yue-Fang, Zhang, Li, Bronfman, Leonardo, Ge, Jixing, Tang, Mengyao, Zhang, Yong, Xu, Feng-Wei, Wang, Yao, Zhou, Bing

المساهمون: University of Helsinki, Department of Physics

مصطلحات موضوعية: stars: formation, ISM: abundances, ISM: individual: G9.62+0.19, ISM: molecules-radio lines: ISM, COMPLEX ORGANIC-MOLECULES, EXTRAORDINARY SOURCES ANALYSIS, HIGH-RESOLUTION OBSERVATIONS, C-12/C-13 ISOTOPE RATIO, WIDE SPECTRAL SURVEY, HOT-CORE, GALACTIC-CENTER, HERSCHEL OBSERVATIONS, IRAS 16293-2422, METHYL FORMATE, Physical sciences

وصف الملف: application/pdf

Relation: This work makes use of the following ALMA data: ADS/JAO.ALMA#2019.1.00685.S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada), 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. This work has been supported by the National Key R&D Program of China (No. 2017YFA0402701), the National Natural Science Foundation of China (NSFC) under grant numbers 12033005 and 11947064, and Yunnan Applied Basic Research Projects under grant no. 202001AU070123. TL acknowledges support by the National Natural Science Foundation of China (NSFC) through grant numbers 12073061 and 12122307, the international partnership programme of Chinese Academy of Sciences through grant no. 114231KYSB20200009, and Shanghai Pujiang Program 20PJ1415500. H-LL is supported by NSFC through grant no. 12103045. GG and LB gratefully acknowledge support from ANID BASAL project FB210003. CWL is supported by the Basic Science Research Program (2019R1A2C1010851) through the National Research Foundation of Korea. DLL acknowledges support from NSFC through grant no. 12173075 and support from the Youth Innovation Promotion Association CAS. KT was supported by JSPS KAKENHI grant no. 20H05645. MT is supported by the scientific research fund project of Yunnan Provincial Education Department (No. 2022J0855). YZ thanks the National Science Foundation of China (NSFC, grant no. 11973099) and acknowledges science research grants from the China Manned Space Project (CMS-CSST-2021-A09 and CMS-CSST-2021-A10) for financial support.; Peng , Y , Liu , T , Qin , S-L , Baug , T , Liu , H-L , Wang , K , Garay , G , Zhang , C , Chen , L-F , Lee , C W , Juvela , M , Li , D , Tatematsu , K , Liu , X-C , Lee , J-E , Luo , G , Dewangan , L , Wu , Y-F , Zhang , L , Bronfman , L , Ge , J , Tang , M , Zhang , Y , Xu , F-W , Wang , Y & Zhou , B 2022 , ' ATOMS : ALMA Three-millimeter Observations of Massive Star-forming regions - X. Chemical differentiation among the massive cores in G9.62+0.19 ' , Monthly Notices of the Royal Astronomical Society , vol. 512 , no. 3 , pp. 4419-4440 . https://doi.org/10.1093/mnras/stac624; ORCID: /0000-0002-5809-4834/work/112286023; http://hdl.handle.net/10138/352554; 86e21895-9602-4e56-83ef-b830acb2d26a; 000779485000007

الاتاحة: http://hdl.handle.net/10138/352554

المؤلفون: Peng, Yaping, Liu, Tie, Qin, Sheng-Li, Baug, Tapas, Liu, Hong-Li, Wang, Ke, Garay Brignardello, Guido Alejandro, Zhang, Chao, Chen, Long-Fei, Lee, Chang Won, Juvela, Mika, Li, Dalei, Tatematsu, Ken'ichi, Liu, Xun-Chuan, Lee, Jeong-Eun, Luo, Gan, Dewangan, Lokesh, Wu, Yue-Fang, Zhang, Li, Bronfman Aguilo, Leonardo Jaime, Ge, Jixing, Tang, Mengyao, Zhang, Yong, Xu, Feng-Wei, Wang, Yao, Zhou, Bing

المصدر: Monthly Notices of the Royal Astronomical Society

مصطلحات موضوعية: ISM:abundances, ISM:individual (G9.62+0.19), ISM:molecules, Radio lines:ISM, Star:formation

وصف الملف: application/pdf

Relation: MNRAS 000, 1–40 (2022); https://repositorio.uchile.cl/handle/2250/186921

الاتاحة: https://doi.org/10.1093/mnras/stac624
https://repositorio.uchile.cl/handle/2250/186921