NAOC Open IR
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 PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume496Issue:3Pages:3668-3687
AbstractScaling 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.
KeywordISM: abundances ISM: dust, extinction galaxies: evolution galaxies: star formation
Funding OrganizationResearch 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)
DOI10.1093/mnras/staa1496
WOS KeywordMASS-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 ProjectResearch 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 OrganizationResearch 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 AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000574919300067
PublisherOXFORD UNIV PRESS
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/81808
Collection中国科学院国家天文台
Corresponding AuthorDe Looze, I
Affiliation1.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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