期刊
ASTROPHYSICAL JOURNAL
卷 868, 期 2, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.3847/1538-4357/aae9f1
关键词
galaxies: abundances; galaxies: evolution; galaxies: starburst; galaxies: star formation
资金
- National Key RAMP
- D Program of China [2015CB857004, 2016YFA0400702, 2017YFA0402600]
- National Natural Science Foundation of China (NSFC) [11320101002, 11421303, 11433005]
- Youth Innovation Fund by the University of Science and Technology of China [WK2030220019]
- China Postdoctoral Science Foundation [BH2030000040]
- National Thousand Young Talents Program of China
- Alfred P. Sloan Foundation
- U.S. Department of Energy Office of Science
- Center for High-Performance Computing at the University of Utah
- Brazilian Participation Group
- Carnegie Institution for Science
- Chilean Participation Group
- French Participation Group
- Harvard-Smithsonian Center for Astrophysics
- Instituto de Astrofisica de Canarias
- Johns Hopkins University
- Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo
- Lawrence Berkeley National Laboratory
- Leibniz Institut fur Astrophysik Potsdam (AIP)
- Max-Planck-Institut fur Astronomie (MPIA Heidelberg)
- Max-Planck-Institut fur Astrophysik (MPA Garching)
- Max-Planck-Institut fur Extraterrestrische Physik (MPE)
- National Astronomical Observatories of China
- New Mexico State University
- New York University
- University of Notre Dame
- Observatrio Nacional/MCTI
- Pennsylvania State University
- Shanghai Astronomical Observatory
- United Kingdom Participation Group
- Universidad Nacional Autonoma de Mexico
- University of Arizona
- University of Colorado Boulder
- University of Oxford
- University of Portsmouth
- University of Utah
- University of Virginia
- University of Washington
- University of Wisconsin
- Vanderbilt University
- Yale University
- Ohio State University
Metallicity and its relationship with other galactic properties is a fundamental probe of the evolution of galaxies. In this work, we select about 750,000 star-forming spatial pixels from 1122 blue galaxies in the Mapping Nearby Galaxies at Apache Point Observatory survey to investigate the global stellar mass-local stellar mass surface density-gas-phase metallicity (M-*-Sigma(*)-Z) relation. At a fixed M*, the metallicity increases steeply with increasing Sigma(*). Similarly, at a fixed Sigma(*), the metallicity increases strongly with increasing M-* at the low-mass end, while this trend becomes less obvious at the high-mass end. We find the metallicity to be more strongly correlated to Sigma(*) than to M-*. Furthermore, we construct a tight (0.07 dex scatter) M-*-Sigma(*)-Z relation, which reduces the scatter in the Sigma(*)-Z relation by about 30% for galaxies with 7.8.
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