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A Universal Fundamental Plane and theM(dyn)-M-* Relation for Galaxies with CALIFA and MaNGA
Aquino-Ortiz, E.1; Sanchez, S. F.1; Valenzuela, O.1; Hernandez-Toledo, H.1; Jin, Yunpeng2; Zhu, Ling3; van de Ven, Glenn4; Barrera-Ballesteros, J. K.1; Avila-Reese, V.1; Rodriguez-Puebla, A.1; Tissera, Patricia B.5
2020-09-01
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume900Issue:2Pages:17
AbstractWe use the stellar kinematics for 2458 galaxies from the MaNGA survey to explore a universal fundamental plane (UFP) described by the equation log (gamma(e)) = log(S-0.5(2)) - log(I-e) - log(R-e) + C, defined by the logarithms of effective radius, R-e; the surface brightness within R-e, I-e; the dynamical mass-to-light ratio within R-e, Y-e; and the total velocity parameter at R-e, S-K(2) = KVRe2 + sigma(2)(*e), where V-Re is the rotation velocity and sigma(*e) is the velocity dispersion. The surface brightness is within R-e, I-e, and the dynamical mass-to-light ratio is within R-e, gamma(e). We use sophisticated Schwarzschild dynamical models for a subsample of 300 galaxies from the CALIFA survey to calibrate the universal fundamental plane. This calibration allows us to propose both (i) a parameterization to estimate the difficult-to-measure averaged dynamical mass-to-light ratio within R-e, gamma(fit)(e), once the internal kinematics, surface brightness, and effective radius are known; and (ii) a new, more robust dynamical mass proxy consistent with dynamical models within 0.09 dex. We reproduce the relation between the dynamical mass and the stellar mass in the inner regions of galaxies with lower scatter. We use the estimated gamma(fit)(e) from our analysis to explore the UFP with the MaNGA data set. We find that all galaxies, from spheroids to disks, follow the UFP with a scatter significantly smaller (0.05 dex) than the one reported for the fundamental plane (similar to 0.09 dex) and comparable with Tully-Fisher studies (similar to 0.05 dex), but for a wider range of galaxy types. We also confirm that spheroidal and spiral galaxies follow the same M-*-S-0.5 scaling relation, with lower scatter than the M-* - V-Re - and M-*-sigma(*e) ones, which is in agreement with previous studies found in the literature.
KeywordGalaxies Early-type galaxies Late-type galaxies Scaling relations Galaxy kinematics
Funding OrganizationCONACYT ; CONACYT ; UNAM ; UNAM ; PAPIIT-DGAPA ; PAPIIT-DGAPA ; European Research Council (ERC) ; European Research Council (ERC) ; Fondecyt ; Fondecyt ; CONICYT ; CONICYT ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center for High-Performance Computing at the University of Utah ; CONACYT ; CONACYT ; UNAM ; UNAM ; PAPIIT-DGAPA ; PAPIIT-DGAPA ; European Research Council (ERC) ; European Research Council (ERC) ; Fondecyt ; Fondecyt ; CONICYT ; CONICYT ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center for High-Performance Computing at the University of Utah ; CONACYT ; CONACYT ; UNAM ; UNAM ; PAPIIT-DGAPA ; PAPIIT-DGAPA ; European Research Council (ERC) ; European Research Council (ERC) ; Fondecyt ; Fondecyt ; CONICYT ; CONICYT ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center for High-Performance Computing at the University of Utah ; CONACYT ; CONACYT ; UNAM ; UNAM ; PAPIIT-DGAPA ; PAPIIT-DGAPA ; European Research Council (ERC) ; European Research Council (ERC) ; Fondecyt ; Fondecyt ; CONICYT ; CONICYT ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center for High-Performance Computing at the University of Utah
DOI10.3847/1538-4357/aba94e
WOS KeywordTULLY-FISHER RELATION ; SDSS-IV MANGA ; POTSDAM MULTIAPERTURE SPECTROPHOTOMETER ; DIGITAL SKY SURVEY ; TO-LIGHT RATIOS ; SCALING RELATIONS ; ELLIPTIC GALAXIES ; DARK-MATTER ; SAURON PROJECT ; STELLAR MASS
Language英语
Funding ProjectCONACYT[CB-285080] ; CONACYT[FC-2016-01-1916] ; UNAM[PAPIIT-DGAPA-IN100519] ; UNAM[IG101620] ; UNAM[PAPIIT-DGAPA-IA100420] ; PAPIIT-DGAPA[IN112518] ; European Research Council (ERC)[724857] ; Fondecyt[1200703] ; CONICYT[AFB-170002] ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah
Funding OrganizationCONACYT ; CONACYT ; UNAM ; UNAM ; PAPIIT-DGAPA ; PAPIIT-DGAPA ; European Research Council (ERC) ; European Research Council (ERC) ; Fondecyt ; Fondecyt ; CONICYT ; CONICYT ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center for High-Performance Computing at the University of Utah ; CONACYT ; CONACYT ; UNAM ; UNAM ; PAPIIT-DGAPA ; PAPIIT-DGAPA ; European Research Council (ERC) ; European Research Council (ERC) ; Fondecyt ; Fondecyt ; CONICYT ; CONICYT ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center for High-Performance Computing at the University of Utah ; CONACYT ; CONACYT ; UNAM ; UNAM ; PAPIIT-DGAPA ; PAPIIT-DGAPA ; European Research Council (ERC) ; European Research Council (ERC) ; Fondecyt ; Fondecyt ; CONICYT ; CONICYT ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center for High-Performance Computing at the University of Utah ; CONACYT ; CONACYT ; UNAM ; UNAM ; PAPIIT-DGAPA ; PAPIIT-DGAPA ; European Research Council (ERC) ; European Research Council (ERC) ; Fondecyt ; Fondecyt ; CONICYT ; CONICYT ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center for High-Performance Computing at the University of Utah
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000570649500001
PublisherIOP PUBLISHING LTD
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/81502
Collection中国科学院国家天文台
Corresponding AuthorAquino-Ortiz, E.
Affiliation1.Univ Nacl Autonoma Mexico, Inst Astron, AP 70-264, Cdmx 04510, Mexico
2.Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100101, Peoples R China
3.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
4.Univ Vienna, Dept Astrophys, TAijrkenschanzstr 17, A-1180 Vienna, Austria
5.Univ Andres Bello, Dept Ciencias Fis, 700 Fernandez Concha, Santiago, Chile
Recommended Citation
GB/T 7714
Aquino-Ortiz, E.,Sanchez, S. F.,Valenzuela, O.,et al. A Universal Fundamental Plane and theM(dyn)-M-* Relation for Galaxies with CALIFA and MaNGA[J]. ASTROPHYSICAL JOURNAL,2020,900(2):17.
APA Aquino-Ortiz, E..,Sanchez, S. F..,Valenzuela, O..,Hernandez-Toledo, H..,Jin, Yunpeng.,...&Tissera, Patricia B..(2020).A Universal Fundamental Plane and theM(dyn)-M-* Relation for Galaxies with CALIFA and MaNGA.ASTROPHYSICAL JOURNAL,900(2),17.
MLA Aquino-Ortiz, E.,et al."A Universal Fundamental Plane and theM(dyn)-M-* Relation for Galaxies with CALIFA and MaNGA".ASTROPHYSICAL JOURNAL 900.2(2020):17.
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