KMS National Astronomical Observatories, CAS
| JINGLE - IV. Dust, HI gas, and metal scaling laws in the local Universe | |
| De Looze, I1,2; Lamperti, I2; Saintonge, A.2; Relano, M.3,4; Smith, M. W. L.5; Clark, C. J. R.6; Wilson, C. D.7; Decleir, M.6; Jones, A. P.8; Kennicutt, R. C.9,10; Accurso, G.2; Brinks, E.11; Bureau, M.12,13,14; Cigan, P.5; Clements, D. L.15; De Vis, P.5; Fanciullo, L.16; Gao, Y.17,18,19; Gear, W. K.20; Ho, L. C.21,22; Hwang, H. S.23; Michalowski, M. J.24; Lee, J. C.23; Li, C.25,26; Lin, L.16; Liu, T.27; Lomaeva, M.2; Pan, H-A16,28; Sargent, M.29; Williams, T.28; Xiao, T.16,30; Zhu, M.31 | |
| 2020-08-01 | |
| Source Publication | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| ISSN | 0035-8711 |
| Volume | 496Issue:3Pages:3668-3687 |
| Abstract | Scaling laws of dust, HI gas, and metal mass with stellar mass, specific star formation rate, and metallicity are crucial to our understanding of the build-up of galaxies through their enrichment with metals and dust. In this work, we analyse how the dust and metal content varies with specific gas mass (M-HI/M-star) across a diverse sample of 423 nearby galaxies. The observed trends are interpreted with a set of Dust and Element evolUtion modelS (DEUS) - including stellar dust production, grain growth, and dust destruction - within a Bayesian framework to enable a rigorous search of the multidimensional parameter space. We find that these scaling laws for galaxies with -1.0 less than or similar to log M-HI/M-star less than or similar to 0 can be reproduced using closed-box models with high fractions (37-89 per cent) of supernova dust surviving a reverse shock, relatively low grain growth efficiencies (subset of = 30-40), and long dust lifetimes (1-2 Gyr). The models have present-day dust masses with similar contributions from stellar sources (50-80 per cent) and grain growth (20-50 per cent). Over the entire lifetime of these galaxies, the contribution from stardust (>90 per cent) outweighs the fraction of dust grown in the interstellar medium (<10 per cent). Our results provide an alternative for the chemical evolution models that require extremely low supernova dust production efficiencies and short grain growth time-scales to reproduce local scaling laws, and could help solving the conundrum on whether or not grains can grow efficiently in the interstellar medium. |
| Keyword | ISM: abundances ISM: dust, extinction galaxies: evolution galaxies: star formation |
| Funding Organization | Research Foundation -Flanders (FWO) ; Research Foundation -Flanders (FWO) ; National Science Foundation of China ; National Science Foundation of China ; National Key RAMP;D Programme of China ; National Key RAMP;D Programme of China ; National Science Centre, Poland through the SONATA BIS grant ; National Science Centre, Poland through the SONATA BIS grant ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; Canada Foundation for Innovation ; JCMT Project ; JCMT Project ; East Asian Observatory ; East Asian Observatory ; BMVIT (Austria) ; BMVIT (Austria) ; ESA-PRODEX (Belgium) ; ESA-PRODEX (Belgium) ; CEA/CNES (France) ; CEA/CNES (France) ; DLR (Germany) ; DLR (Germany) ; ASI/INAF (Italy) ; ASI/INAF (Italy) ; CICYT/MCYT (Spain) ; CICYT/MCYT (Spain) ; CSA (Canada) ; CSA (Canada) ; NAOC (China) ; NAOC (China) ; CEA (France) ; CEA (France) ; CNES (France) ; CNES (France) ; CNRS (France) ; CNRS (France) ; ASI (Italy) ; ASI (Italy) ; MCINN (Spain) ; MCINN (Spain) ; SNSB (Sweden) ; SNSB (Sweden) ; STFC (UK) ; STFC (UK) ; UKSA (UK) ; UKSA (UK) ; NASA (USA) ; NASA (USA) ; Research Foundation -Flanders (FWO) ; Research Foundation -Flanders (FWO) ; National Science Foundation of China ; National Science Foundation of China ; National Key RAMP;D Programme of China ; National Key RAMP;D Programme of China ; National Science Centre, Poland through the SONATA BIS grant ; National Science Centre, Poland through the SONATA BIS grant ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; Canada Foundation for Innovation ; JCMT Project ; JCMT Project ; East Asian Observatory ; East Asian Observatory ; BMVIT (Austria) ; BMVIT (Austria) ; ESA-PRODEX (Belgium) ; ESA-PRODEX (Belgium) ; CEA/CNES (France) ; CEA/CNES (France) ; DLR (Germany) ; DLR (Germany) ; ASI/INAF (Italy) ; ASI/INAF (Italy) ; CICYT/MCYT (Spain) ; CICYT/MCYT (Spain) ; CSA (Canada) ; CSA (Canada) ; NAOC (China) ; NAOC (China) ; CEA (France) ; CEA (France) ; CNES (France) ; CNES (France) ; CNRS (France) ; CNRS (France) ; ASI (Italy) ; ASI (Italy) ; MCINN (Spain) ; MCINN (Spain) ; SNSB (Sweden) ; SNSB (Sweden) ; STFC (UK) ; STFC (UK) ; UKSA (UK) ; UKSA (UK) ; NASA (USA) ; NASA (USA) ; Research Foundation -Flanders (FWO) ; Research Foundation -Flanders (FWO) ; National Science Foundation of China ; National Science Foundation of China ; National Key RAMP;D Programme of China ; National Key RAMP;D Programme of China ; National Science Centre, Poland through the SONATA BIS grant ; National Science Centre, Poland through the SONATA BIS grant ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; Canada Foundation for Innovation ; JCMT Project ; JCMT Project ; East Asian Observatory ; East Asian Observatory ; BMVIT (Austria) ; BMVIT (Austria) ; ESA-PRODEX (Belgium) ; ESA-PRODEX (Belgium) ; CEA/CNES (France) ; CEA/CNES (France) ; DLR (Germany) ; DLR (Germany) ; ASI/INAF (Italy) ; ASI/INAF (Italy) ; CICYT/MCYT (Spain) ; CICYT/MCYT (Spain) ; CSA (Canada) ; CSA (Canada) ; NAOC (China) ; NAOC (China) ; CEA (France) ; CEA (France) ; CNES (France) ; CNES (France) ; CNRS (France) ; CNRS (France) ; ASI (Italy) ; ASI (Italy) ; MCINN (Spain) ; MCINN (Spain) ; SNSB (Sweden) ; SNSB (Sweden) ; STFC (UK) ; STFC (UK) ; UKSA (UK) ; UKSA (UK) ; NASA (USA) ; NASA (USA) ; Research Foundation -Flanders (FWO) ; Research Foundation -Flanders (FWO) ; National Science Foundation of China ; National Science Foundation of China ; National Key RAMP;D Programme of China ; National Key RAMP;D Programme of China ; National Science Centre, Poland through the SONATA BIS grant ; National Science Centre, Poland through the SONATA BIS grant ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; Canada Foundation for Innovation ; JCMT Project ; JCMT Project ; East Asian Observatory ; East Asian Observatory ; BMVIT (Austria) ; BMVIT (Austria) ; ESA-PRODEX (Belgium) ; ESA-PRODEX (Belgium) ; CEA/CNES (France) ; CEA/CNES (France) ; DLR (Germany) ; DLR (Germany) ; ASI/INAF (Italy) ; ASI/INAF (Italy) ; CICYT/MCYT (Spain) ; CICYT/MCYT (Spain) ; CSA (Canada) ; CSA (Canada) ; NAOC (China) ; NAOC (China) ; CEA (France) ; CEA (France) ; CNES (France) ; CNES (France) ; CNRS (France) ; CNRS (France) ; ASI (Italy) ; ASI (Italy) ; MCINN (Spain) ; MCINN (Spain) ; SNSB (Sweden) ; SNSB (Sweden) ; STFC (UK) ; STFC (UK) ; UKSA (UK) ; UKSA (UK) ; NASA (USA) ; NASA (USA) |
| DOI | 10.1093/mnras/staa1496 |
| WOS Keyword | MASS-METALLICITY RELATION ; STAR-FORMING GALAXIES ; JCMT LEGACY SURVEY ; NEARBY GALAXIES ; STELLAR MASS ; ABSORPTION-COEFFICIENT ; FORMATION HISTORY ; HERSCHEL-ATLAS ; EMISSION-LINE ; MOLECULAR GAS |
| Language | 英语 |
| Funding Project | Research Foundation -Flanders (FWO) ; National Science Foundation of China[11721303] ; National Key RAMP;D Programme of China[2016YFA0400702] ; National Science Centre, Poland through the SONATA BIS grant[2018/30/E/ST9/00208] ; Chinese Academy of Sciences[XDB09000000] ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; JCMT Project[M16AL005] ; East Asian Observatory ; BMVIT (Austria) ; ESA-PRODEX (Belgium) ; CEA/CNES (France) ; DLR (Germany) ; ASI/INAF (Italy) ; CICYT/MCYT (Spain) ; CSA (Canada) ; NAOC (China) ; CEA (France) ; CNES (France) ; CNRS (France) ; ASI (Italy) ; MCINN (Spain) ; SNSB (Sweden) ; STFC (UK) ; UKSA (UK) ; NASA (USA) |
| Funding Organization | Research Foundation -Flanders (FWO) ; Research Foundation -Flanders (FWO) ; National Science Foundation of China ; National Science Foundation of China ; National Key RAMP;D Programme of China ; National Key RAMP;D Programme of China ; National Science Centre, Poland through the SONATA BIS grant ; National Science Centre, Poland through the SONATA BIS grant ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; Canada Foundation for Innovation ; JCMT Project ; JCMT Project ; East Asian Observatory ; East Asian Observatory ; BMVIT (Austria) ; BMVIT (Austria) ; ESA-PRODEX (Belgium) ; ESA-PRODEX (Belgium) ; CEA/CNES (France) ; CEA/CNES (France) ; DLR (Germany) ; DLR (Germany) ; ASI/INAF (Italy) ; ASI/INAF (Italy) ; CICYT/MCYT (Spain) ; CICYT/MCYT (Spain) ; CSA (Canada) ; CSA (Canada) ; NAOC (China) ; NAOC (China) ; CEA (France) ; CEA (France) ; CNES (France) ; CNES (France) ; CNRS (France) ; CNRS (France) ; ASI (Italy) ; ASI (Italy) ; MCINN (Spain) ; MCINN (Spain) ; SNSB (Sweden) ; SNSB (Sweden) ; STFC (UK) ; STFC (UK) ; UKSA (UK) ; UKSA (UK) ; NASA (USA) ; NASA (USA) ; Research Foundation -Flanders (FWO) ; Research Foundation -Flanders (FWO) ; National Science Foundation of China ; National Science Foundation of China ; National Key RAMP;D Programme of China ; National Key RAMP;D Programme of China ; National Science Centre, Poland through the SONATA BIS grant ; National Science Centre, Poland through the SONATA BIS grant ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; Canada Foundation for Innovation ; JCMT Project ; JCMT Project ; East Asian Observatory ; East Asian Observatory ; BMVIT (Austria) ; BMVIT (Austria) ; ESA-PRODEX (Belgium) ; ESA-PRODEX (Belgium) ; CEA/CNES (France) ; CEA/CNES (France) ; DLR (Germany) ; DLR (Germany) ; ASI/INAF (Italy) ; ASI/INAF (Italy) ; CICYT/MCYT (Spain) ; CICYT/MCYT (Spain) ; CSA (Canada) ; CSA (Canada) ; NAOC (China) ; NAOC (China) ; CEA (France) ; CEA (France) ; CNES (France) ; CNES (France) ; CNRS (France) ; CNRS (France) ; ASI (Italy) ; ASI (Italy) ; MCINN (Spain) ; MCINN (Spain) ; SNSB (Sweden) ; SNSB (Sweden) ; STFC (UK) ; STFC (UK) ; UKSA (UK) ; UKSA (UK) ; NASA (USA) ; NASA (USA) ; Research Foundation -Flanders (FWO) ; Research Foundation -Flanders (FWO) ; National Science Foundation of China ; National Science Foundation of China ; National Key RAMP;D Programme of China ; National Key RAMP;D Programme of China ; National Science Centre, Poland through the SONATA BIS grant ; National Science Centre, Poland through the SONATA BIS grant ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; Canada Foundation for Innovation ; JCMT Project ; JCMT Project ; East Asian Observatory ; East Asian Observatory ; BMVIT (Austria) ; BMVIT (Austria) ; ESA-PRODEX (Belgium) ; ESA-PRODEX (Belgium) ; CEA/CNES (France) ; CEA/CNES (France) ; DLR (Germany) ; DLR (Germany) ; ASI/INAF (Italy) ; ASI/INAF (Italy) ; CICYT/MCYT (Spain) ; CICYT/MCYT (Spain) ; CSA (Canada) ; CSA (Canada) ; NAOC (China) ; NAOC (China) ; CEA (France) ; CEA (France) ; CNES (France) ; CNES (France) ; CNRS (France) ; CNRS (France) ; ASI (Italy) ; ASI (Italy) ; MCINN (Spain) ; MCINN (Spain) ; SNSB (Sweden) ; SNSB (Sweden) ; STFC (UK) ; STFC (UK) ; UKSA (UK) ; UKSA (UK) ; NASA (USA) ; NASA (USA) ; Research Foundation -Flanders (FWO) ; Research Foundation -Flanders (FWO) ; National Science Foundation of China ; National Science Foundation of China ; National Key RAMP;D Programme of China ; National Key RAMP;D Programme of China ; National Science Centre, Poland through the SONATA BIS grant ; National Science Centre, Poland through the SONATA BIS grant ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; Canada Foundation for Innovation ; JCMT Project ; JCMT Project ; East Asian Observatory ; East Asian Observatory ; BMVIT (Austria) ; BMVIT (Austria) ; ESA-PRODEX (Belgium) ; ESA-PRODEX (Belgium) ; CEA/CNES (France) ; CEA/CNES (France) ; DLR (Germany) ; DLR (Germany) ; ASI/INAF (Italy) ; ASI/INAF (Italy) ; CICYT/MCYT (Spain) ; CICYT/MCYT (Spain) ; CSA (Canada) ; CSA (Canada) ; NAOC (China) ; NAOC (China) ; CEA (France) ; CEA (France) ; CNES (France) ; CNES (France) ; CNRS (France) ; CNRS (France) ; ASI (Italy) ; ASI (Italy) ; MCINN (Spain) ; MCINN (Spain) ; SNSB (Sweden) ; SNSB (Sweden) ; STFC (UK) ; STFC (UK) ; UKSA (UK) ; UKSA (UK) ; NASA (USA) ; NASA (USA) |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000574919300067 |
| Publisher | OXFORD UNIV PRESS |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.bao.ac.cn/handle/114a11/81812 |
| Collection | 中国科学院国家天文台 |
| Corresponding Author | De Looze, I |
| Affiliation | 1.Univ Ghent, Sterrenkundig Observ, Krijgslaan 281-S9, B-9000 Ghent, Belgium 2.UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England 3.Univ Granada, Dept Fis Teor & Cosmos, E-18071 Granada, Spain 4.Univ Granada, Inst Univ Carlos I Fis Teor & Computac, E-18071 Granada, Spain 5.Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, Wales 6.Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21211 USA 7.McMaster Univ, Dept Phys & Astron, Hamilton, ON L8S 4M1, Canada 8.Univ Paris Saclay, Inst Astrophys Spatiale, CNRS, F-91405 Orsay, France 9.Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA 10.Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, College Stn, TX 77843 USA 11.Univ Hertfordshire, Ctr Astrophys Res, Coll Lane, Hatfield AL10 9AB, Herts, England 12.Univ Oxford, Subdept Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England 13.Yonsei Univ, Yonsei Frontier Lab, 50 Yonsei Ro, Seoul 03722, South Korea 14.Yonsei Univ, Dept Astron, 50 Yonsei Ro, Seoul 03722, South Korea 15.Imperial Coll, Phys Dept, Blacken Lab, London SW7 2AZ, England 16.Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan 17.Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China 18.Chinese Acad Sci, Purple Mt Observ, Nanjing 210034, Peoples R China 19.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210034, Peoples R China 20.Natl Univ Ireland, Ctr Astron, Univ Rd, Galway H91 TK33, Ireland 21.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 22.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China 23.Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea 24.Adam Mickiewicz Univ, Fac Phys, Astron Observ Inst, Ul Sloneczna 36, PL-60286 Poznan, Poland 25.Tsinghua Univ, Tsinghua Ctr Astrophys, Beijing 100084, Peoples R China 26.Tsinghua Univ, Phys Dept, Beijing 100084, Peoples R China 27.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China 28.Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany 29.Univ Sussex, Astron Ctr, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England 30.Zhejiang Univ, Dept Phys, Hangzhou 310027, Zhejiang, Peoples R China 31.Natl Astron Observ China, 20A Datun Rd, Beijing 100012, Peoples R China |
| Recommended Citation GB/T 7714 | De Looze, I,Lamperti, I,Saintonge, A.,et al. JINGLE - IV. Dust, HI gas, and metal scaling laws in the local Universe[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2020,496(3):3668-3687. |
| APA | De Looze, I.,Lamperti, I.,Saintonge, A..,Relano, M..,Smith, M. W. L..,...&Zhu, M..(2020).JINGLE - IV. Dust, HI gas, and metal scaling laws in the local Universe.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,496(3),3668-3687. |
| MLA | De Looze, I,et al."JINGLE - IV. Dust, HI gas, and metal scaling laws in the local Universe".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 496.3(2020):3668-3687. |
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