NAOC Open IR
The Fornax 3D project: PNe populations and stellar metallicity in edge-on galaxies
Galan-de Anta, P. M.1,2; Sarzi, M.1,3; Spriggs, T. W.3; Nedelchev, B.1,3; Pinna, F.4; Martin-Navarro, I.4,5,6; Coccato, L.7; Corsini, E. M.8,9; de Zeeuw, P. T.10,11; Falcon-Barroso, J.5,6; Gadotti, D. A.7; Iodice, E.7,12; Fahrion, K.7; Lyubenova, M.7; McDermid, R. M.13,14; Morelli, L.15; van de Ven, G.16; Viaene, S.17; Zhu, L.18
2021-08-19
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume652Pages:7
AbstractContext. Extragalactic planetary nebulae (PNe) are useful distance indicators and are often used to trace the dark-matter content in external galaxies. At the same time, PNe can also be used as probes of their host galaxy stellar populations and to help understand the later stages of stellar evolution. Previous works have indicated that a specific number of PNe per stellar luminosity can vary across different galaxies and as a function of stellar-population properties, for instance increasing with decreasing stellar metallicity. Aims. In this study we further explore the importance of stellar metallicity in driving the properties of the PNe population in early-type galaxies, using three edge-on galaxies in the Fornax cluster offering a clear view into their predominantly metal-rich and metal-poor regions near the equatorial plane or both below and above it, respectively. Methods. Using very large telescope-multi unit spectroscopic explorer (VLT-MUSE) integral-field observations and dedicated PNe detection procedures, we constructed the PNe luminosity function and computed the luminosity-specific number of PNe alpha in both in- and off-plane regions of our edge-on systems. Results. Comparing these alpha values with metallicity measurements also based on the same MUSE data, we find no evidence for an increase in the specific abundance of PNe when transitioning between metal-rich and metal-poor regions. Conclusions. Our analysis highlights the importance of ensuring spatial consistency to avoid misleading results when investigating the link between PNe and their parent stellar populations, and suggest that in passively evolving systems variations in the specific number of PNe may pertain to rather extreme metallicity regimes found either in the innermost or outermost regions of galaxies.
Keywordplanetary nebulae: general galaxies: abundances galaxies: elliptical and lenticular, cD techniques: imaging spectroscopy methods: observational
Funding OrganizationScience and Technology Facilities Council ; Science and Technology Facilities Council ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; IAC project TRACES ; IAC project TRACES ; Padua University ; Padua University ; MIUR ; MIUR ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Science and Technology Facilities Council ; Science and Technology Facilities Council ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; IAC project TRACES ; IAC project TRACES ; Padua University ; Padua University ; MIUR ; MIUR ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Science and Technology Facilities Council ; Science and Technology Facilities Council ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; IAC project TRACES ; IAC project TRACES ; Padua University ; Padua University ; MIUR ; MIUR ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Science and Technology Facilities Council ; Science and Technology Facilities Council ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; IAC project TRACES ; IAC project TRACES ; Padua University ; Padua University ; MIUR ; MIUR ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community
DOI10.1051/0004-6361/202140834
WOS KeywordPLANETARY-NEBULAE POPULATION ; ATLAS(3D) PROJECT ; STANDARD CANDLES ; EVOLUTION ; VELOCITY ; CLUSTER ; DYNAMICS ; SPECTRA ; REGIONS ; STARS
Language英语
Funding ProjectScience and Technology Facilities Council[ST/R504786/1] ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU)[PID2019-107427GB-C32] ; IAC project TRACES ; Padua University[DOR1885254/18] ; Padua University[DOR1935272/19] ; Padua University[DOR2013080/20] ; MIUR[PRIN 2017 20173ML3WW001] ; European Research Council (ERC) under the European Union[724857] ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community
Funding OrganizationScience and Technology Facilities Council ; Science and Technology Facilities Council ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; IAC project TRACES ; IAC project TRACES ; Padua University ; Padua University ; MIUR ; MIUR ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Science and Technology Facilities Council ; Science and Technology Facilities Council ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; IAC project TRACES ; IAC project TRACES ; Padua University ; Padua University ; MIUR ; MIUR ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Science and Technology Facilities Council ; Science and Technology Facilities Council ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; IAC project TRACES ; IAC project TRACES ; Padua University ; Padua University ; MIUR ; MIUR ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Science and Technology Facilities Council ; Science and Technology Facilities Council ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; RAVET project from the Spanish Ministry of Science, Innovation and Universities (MCIU) ; IAC project TRACES ; IAC project TRACES ; Padua University ; Padua University ; MIUR ; MIUR ; European Research Council (ERC) under the European Union ; European Research Council (ERC) under the European Union ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community ; Consejeria de Economia, Industria, Comercio y Conocimiento of the Canary Islands Autonomous Community
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000686300800004
PublisherEDP SCIENCES S A
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/75352
Collection中国科学院国家天文台
Corresponding AuthorGalan-de Anta, P. M.
Affiliation1.Armagh Observ & Planetarium, Coll Hill, Armagh BT61 9DG, North Ireland
2.Queens Univ Belfast, Sch Math & Phys, Astrophys Res Ctr, Belfast BT7 INN, Antrim, North Ireland
3.Univ Hertfordshire, Ctr Astrophys Res, Coll Lane, Hatfield AL10 9AB, Herts, England
4.Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany
5.Inst Astrofis Canarias, Via Lactea S-N, San Cristobal la Laguna 38205, Tenerife, Spain
6.Univ La Laguna, Dept Astrofis, Calle Astrofis Francisco Sanchez S-N, San Cristobal la Laguna 38206, Tenerife, Spain
7.European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany
8.Univ Padua, Dipartimento Fis & Astron G Galilei, Vicolo Osservatorio 3, I-35122 Padua, Italy
9.INAF, Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy
10.Leiden Univ, Sterrewacht Leiden, Postbus 9513, NL-2300 RA Leiden, Netherlands
11.Max Planck Inst Extraterr Phys, Giessenbachstr, D-85741 Garching, Germany
12.INAF, Astron Observ Capodimonte, Salita Moiariello 16, I-80131 Naples, Italy
13.Macquarie Univ, Dept Phys & Astron, Sydney, NSW 2109, Australia
14.ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Sydney, NSW, Australia
15.Univ Atacama, Inst Astron & Ciencias Planetarias, Ave Copayapu 485, Copiapo, Chile
16.Univ Vienna, Dept Astrophys, Turkenschanzstr 17, A-1180 Vienna, Austria
17.Univ Ghent, Sterrenkundig Observ, Krijgslaan 281, B-9000 Ghent, Belgium
18.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
Recommended Citation
GB/T 7714
Galan-de Anta, P. M.,Sarzi, M.,Spriggs, T. W.,et al. The Fornax 3D project: PNe populations and stellar metallicity in edge-on galaxies[J]. ASTRONOMY & ASTROPHYSICS,2021,652:7.
APA Galan-de Anta, P. M..,Sarzi, M..,Spriggs, T. W..,Nedelchev, B..,Pinna, F..,...&Zhu, L..(2021).The Fornax 3D project: PNe populations and stellar metallicity in edge-on galaxies.ASTRONOMY & ASTROPHYSICS,652,7.
MLA Galan-de Anta, P. M.,et al."The Fornax 3D project: PNe populations and stellar metallicity in edge-on galaxies".ASTRONOMY & ASTROPHYSICS 652(2021):7.
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