NAOC Open IR
The CALIFA view on stellar angular momentum across the Hubble sequence
Falcon-Barroso, J.1,2; van de Ven, G.3; Lyubenova, M.4; Mendez-Abreu, J.1,2; Aguerri, J. A. L.1,2; Garcia-Lorenzo, B.1,2; Bekeraite, S.5; Sanchez, S. F.6; Husemann, B.7; Garcia-Benito, R.8; Gonzalez Delgado, R. M.8; Mast, D.9,10; Walcher, C. J.5; Zibetti, S.11; Zhu, L.12; Barrera-Ballesteros, J. K.6; Galbany, L.13; Sanchez-Blazquez, P.14; Singh, R.7; van den Bosch, R. C. E.7; Wild, V15; Bland-Hawthorn, J.16,17; Cid Fernandes, R.18; de Lorenzo-Caceres, A.1,2; Gallazzi, A.11; Marino, R. A.19; Marquez, I8; Peletier, R. F.20; Perez, E.8; Perez, I21,22; Roth, M. M.5; Rosales-Ortega, F. F.23; Ruiz-Lara, T.1,2; Wisotzki, L.5; Ziegler, B.3
2019-11-28
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume632Pages:17
AbstractWe present the apparent stellar angular momentum over the optical extent of 300 galaxies across the Hubble sequence using integral-field spectroscopic (IFS) data from the CALIFA survey. Adopting the same lambda(R) parameter previously used to distinguish between slow and fast rotating early-type (elliptical and lenticular) galaxies, we show that spiral galaxies are almost all fast rotators, as expected. Given the extent of our data, we provide relations for lambda(R) measured in different apertures (e.g. fractions of the effective radius: 0.5 R-e, R-e, 2 R-e), including conversions to long-slit 1D apertures. Our sample displays a wide range of lambda(Re) values, consistent with previous IFS studies. The fastest rotators are dominated by relatively massive and highly star-forming Sb galaxies, which preferentially reside in the main star-forming sequence. These galaxies reach lambda(Re) values of similar to 0.85, and they are the largest galaxies at a given mass, while also displaying some of the strongest stellar population gradients. Compared to the population of S0 galaxies, our findings suggest that fading may not be the dominant mechanism transforming spirals into lenticulars. Interestingly, we find that lambda(Re) decreases for late-type Sc and Sd spiral galaxies, with values that occasionally set them in the slow-rotator regime. While for some of them this can be explained by their irregular morphologies and/or face-on configurations, others are edge-on systems with no signs of significant dust obscuration. The latter are typically at the low-mass end, but this does not explain their location in the classical (V/sigma,epsilon) and (lambda(Re), epsilon) diagrams. Our initial investigations, based on dynamical models, suggest that these are dynamically hot disks, probably influenced by the observed important fraction of dark matter within R-e.
Keywordgalaxies: kinematics and dynamics galaxies: elliptical and lenticular, cD galaxies: spiral galaxies: structure galaxies: evolution galaxies: formation
Funding OrganizationSpanish Ministry of Economy and Competitiveness (MINECO) ; Spanish Ministry of Economy and Competitiveness (MINECO) ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; European Regional Development Fund (FEDER) ; European Regional Development Fund (FEDER) ; CONACYT ; CONACYT ; UNAM ; UNAM ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; US National Science Foundation ; US National Science Foundation ; Junta de Andaluci a FQ1580 ; Junta de Andaluci a FQ1580 ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; Spanish Ministry of Economy and Competitiveness (MINECO) ; Spanish Ministry of Economy and Competitiveness (MINECO) ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; European Regional Development Fund (FEDER) ; European Regional Development Fund (FEDER) ; CONACYT ; CONACYT ; UNAM ; UNAM ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; US National Science Foundation ; US National Science Foundation ; Junta de Andaluci a FQ1580 ; Junta de Andaluci a FQ1580 ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; Spanish Ministry of Economy and Competitiveness (MINECO) ; Spanish Ministry of Economy and Competitiveness (MINECO) ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; European Regional Development Fund (FEDER) ; European Regional Development Fund (FEDER) ; CONACYT ; CONACYT ; UNAM ; UNAM ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; US National Science Foundation ; US National Science Foundation ; Junta de Andaluci a FQ1580 ; Junta de Andaluci a FQ1580 ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; Spanish Ministry of Economy and Competitiveness (MINECO) ; Spanish Ministry of Economy and Competitiveness (MINECO) ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; European Regional Development Fund (FEDER) ; European Regional Development Fund (FEDER) ; CONACYT ; CONACYT ; UNAM ; UNAM ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; US National Science Foundation ; US National Science Foundation ; Junta de Andaluci a FQ1580 ; Junta de Andaluci a FQ1580 ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award
DOI10.1051/0004-6361/201936413
WOS KeywordEARLY-TYPE GALAXIES ; INTEGRAL-FIELD SPECTROSCOPY ; SDSS-IV MANGA ; ATLAS(3D) PROJECT ; SAURON PROJECT ; DWARF ELLIPTICALS ; STAR-FORMATION ; VIRGO CLUSTER ; POPULATION SYNTHESIS ; SIMULATED GALAXIES
Language英语
Funding ProjectSpanish Ministry of Economy and Competitiveness (MINECO)[AYA2016-77237-C3-1-P] ; European Research Council (ERC) under the European Union[724857] ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; European Regional Development Fund (FEDER)[AYA2015-68217-P] ; CONACYT[CB-285080] ; CONACYT[FC-2016-01-1916] ; UNAM[PAPIIT-DGAPA-IA101217] ; Shanghai Astronomical Observatory, Chinese Academy of Sciences[Y895201009] ; US National Science Foundation[AST-1311862] ; Junta de Andaluci a FQ1580 ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award[SEV-2017-0709] ; [AYA2016-77846-P] ; [AYA2014-57490-P] ; [AYA2010-15081] ; [AYA2013-42227-P] ; [AYA2016-76682-C3-1-P]
Funding OrganizationSpanish Ministry of Economy and Competitiveness (MINECO) ; Spanish Ministry of Economy and Competitiveness (MINECO) ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; European Regional Development Fund (FEDER) ; European Regional Development Fund (FEDER) ; CONACYT ; CONACYT ; UNAM ; UNAM ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; US National Science Foundation ; US National Science Foundation ; Junta de Andaluci a FQ1580 ; Junta de Andaluci a FQ1580 ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; Spanish Ministry of Economy and Competitiveness (MINECO) ; Spanish Ministry of Economy and Competitiveness (MINECO) ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; European Regional Development Fund (FEDER) ; European Regional Development Fund (FEDER) ; CONACYT ; CONACYT ; UNAM ; UNAM ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; US National Science Foundation ; US National Science Foundation ; Junta de Andaluci a FQ1580 ; Junta de Andaluci a FQ1580 ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; Spanish Ministry of Economy and Competitiveness (MINECO) ; Spanish Ministry of Economy and Competitiveness (MINECO) ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; European Regional Development Fund (FEDER) ; European Regional Development Fund (FEDER) ; CONACYT ; CONACYT ; UNAM ; UNAM ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; US National Science Foundation ; US National Science Foundation ; Junta de Andaluci a FQ1580 ; Junta de Andaluci a FQ1580 ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; Spanish Ministry of Economy and Competitiveness (MINECO) ; Spanish Ministry of Economy and Competitiveness (MINECO) ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) ; European Regional Development Fund (FEDER) ; European Regional Development Fund (FEDER) ; CONACYT ; CONACYT ; UNAM ; UNAM ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; Shanghai Astronomical Observatory, Chinese Academy of Sciences ; US National Science Foundation ; US National Science Foundation ; Junta de Andaluci a FQ1580 ; Junta de Andaluci a FQ1580 ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000514935000001
PublisherEDP SCIENCES S A
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/54298
Collection中国科学院国家天文台
Corresponding AuthorFalcon-Barroso, J.
Affiliation1.Inst Astrofis Canarias, Via Lactea S-N, Tenerife 38205, Spain
2.Univ La Laguna, Dept Astrofis, Tenerife 38205, Spain
3.Univ Vienna, Dept Astrophys, Turkenschanzstr 17, A-1180 Vienna, Austria
4.European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany
5.Leibniz Inst Astrophys Potsdam AlP, Sternwarte 16, D-14482 Potsdam, Germany
6.Univ Nacl Autonoma Mexico, Inst Astron, Apartado Postal 70-264, Mexico City 04510, DF, Mexico
7.Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany
8.CSIC, IAA, Glorieta Astron S-N Aptdo, E-18080 Granada, Spain
9.Observ Astron, Laprida 854,X5000BGR, Cordoba, Argentina
10.Consejo Invest Cient & Tecn Republ Argentina, Avda Rivadavia 1917,C1033AAJ, Caba, Argentina
11.Osserv Astrofis Arcetri, INAF, I-50125 Florence, Italy
12.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
13.Univ Pittsburgh, Dept Phys & Astron, PITT PACC, Pittsburgh, PA 15260 USA
14.Univ Autonoma Madrid, Dept Fis Teor, E-28049 Madrid, Spain
15.Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
16.Univ Sydney, Sydney Inst Astron, Sch Phys A28, Sydney, NSW 2006, Australia
17.ARC Ctr Excellence All Sky Astrophys 3D ASTRO 3D, Crawley, WA, Australia
18.Univ Fed Santa Catarina, Dept Fis, POB 476, BR-88040900 Florianopolis, SC, Brazil
19.Swiss Fed Inst Technol, Inst Astron, Wolfgang Pauli Str 27, CH-8093 Zurich, Switzerland
20.Univ Groningen, Kapteyn Astron Inst, Postbus 800, NL-9700 Groningen, Netherlands
21.Univ Granada, Dept Fis Teor & Cosmos, Fac Ciencias, Edificio Mecenas, E-18071 Granada, Spain
22.Inst Carlos I Fis Teor & Computac, Seville, Spain
23.Inst Nacl Astrofis Opt & Electr, Luis E Erro 1, Puebla 72840, Mexico
Recommended Citation
GB/T 7714
Falcon-Barroso, J.,van de Ven, G.,Lyubenova, M.,et al. The CALIFA view on stellar angular momentum across the Hubble sequence[J]. ASTRONOMY & ASTROPHYSICS,2019,632:17.
APA Falcon-Barroso, J..,van de Ven, G..,Lyubenova, M..,Mendez-Abreu, J..,Aguerri, J. A. L..,...&Ziegler, B..(2019).The CALIFA view on stellar angular momentum across the Hubble sequence.ASTRONOMY & ASTROPHYSICS,632,17.
MLA Falcon-Barroso, J.,et al."The CALIFA view on stellar angular momentum across the Hubble sequence".ASTRONOMY & ASTROPHYSICS 632(2019):17.
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