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The first view of delta Scuti and gamma Doradus stars with the TESS mission
Antoci, V.1; Cunha, M. S.2; Bowman, D. M.3; Murphy, S. J.1,4; Kurtz, D. W.5; Bedding, T. R.1,4; Borre, C. C.1; Christophe, S.6; Daszynska-Daszkiewicz, J.7; Fox-Machado, L.8; Hernandez, A. Garcia9,10; Ghasemi, H.11; Handberg, R.1; Hansen, H.1; Hasanzadeh, A.12; Houdek, G.1; Johnston, C.3; Justesen, A. B.1; Alicavus, F. Kahraman13,14; Kotysz, K.7; Latham, D.15; Matthews, J. M.16; Monster, J.1; Niemczura, E.7; Paunzen, E.17; Arias, J. P. Sanchez18; Pigulski, A.7; Pepper, J.19; Richey-Yowell, T.19,20; Safari, H.12; Seager, S.21,22,23; Smalley, B.24; Shutt, T.25; Sodor, A.26,27; Suarez, J. -C.9,10; Tkachenko, A.3; Wu T(吴涛)28,29,30; Zwintz, K.31; Forteza, S. Barcelo32; Brunsden, E.25; Bognar, Z.26,27; Buzasi, D. L.33; Chowdhury, S.13; De Cat, P.34; Evans, J. A.24; Guo, Z.13,35; Guzik, J. A.36; Jevtic, N.37; Lampens, P.34; Martiz, M. Lares10; Lovekin, C.38; Li, G.4; Mirouh, G. M.39; Mkrtichian, D.40; Monteiro, M. J. P. F. G.2,41; Nemec, J. M.42; Ouazzani, R. -M.6; Pascual-Granado, J.10; Reese, D. R.6; Rieutord, M.43; Rodon, J. R.10; Skarka, M.44,45; Sowicka, P.13; Stateva, I.46; Szabo, R.26,27; Weiss, W. W.47
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2019-12-01
卷号490期号:3页码:4040-4059
DOI10.1093/mnras/stz2787
产权排序第28完成单位
收录类别SCI ; EI
关键词asteroseismology techniques: photometric stars: chemically peculiar stars: interiors stars: variables: delta Scuti
摘要

We present the first asteroseismic results for delta Scuti and gamma Doradus stars observed in Sectors 1 and 2 of the TESS mission. We utilize the 2-min cadence TESS data for a sample of 117 stars to classify their behaviour regarding variability and place them in the Hertzsprung-Russell diagram using Gaia DR2 data. Included within our sample are the eponymous members of two pulsator classes, gamma Doradus and SX Phoenicis. Our sample of pulsating intermediate-mass stars observed by TESS also allows us to confront theoretical models of pulsation driving in the classical instability strip for the first time and show that mixing processes in the outer envelope play an important role. We derive an empirical estimate of 74 per cent for the relative amplitude suppression factor as a result of the redder TESS passband compared to the Kepler mission using a pulsating eclipsing binary system. Furthermore, our sample contains many high-frequency pulsators, allowing us to probe the frequency variability of hot young d Scuti stars, which were lacking in the Kepler mission data set, and identify promising targets for future asteroseismic modelling. The TESS data also allow us to refine the stellar parameters of SX Phoenicis, which is believed to be a blue straggler.

资助项目NASA Explorer Program ; Danish National Re-search Foundation[DNRF106] ; ESA PRODEX[PEA 4000119301] ; Stellar Astrophysics Centre (SAC) at Aarhus University ; NASA[NAS5-2655] ; Danish National Research Foundation[DNRF106] ; FCT -Fundacao para a Ciencia e a Tecnologia ; FEDER through COMPETE2020 -Programa Operacional Competitividade e Internacionalizacao[UID/FIS/04434/2019] ; FEDER through COMPETE2020 -Programa Operacional Competitividade e Internacionalizacao[PTDC/FIS-AST/30389/2017] ; FEDER through COMPETE2020 -Programa Operacional Competitividade e Internacionalizacao[POCI-01-0145-FEDER-030389] ; FCT[CEECIND/02619/2017] ; Polish National Science Center (NCN)[2018/29/B/ST9/02803] ; Polish National Science Center (NCN)[2015/18/A/ST9/00578] ; Polish National Science Center (NCN)[2016/21/B/ST9/01126] ; Spanish public funds under Spanish Ministry of Science and Education[ESP201787676-2-2] ; Spanish public funds under Spanish Ministry of Science and Education[ESP2015-65712-C5-5-R] ; NSF REU program[PHY-1359195] ; Lendulet Program of the Hungarian Academy of Sciences[LP2018-7/2018] ; National Research, Development and Innovation Fund of Hungary under the K16 funding scheme[115709] ; Spanish public funds[ESP2015-65712-C5-5-R] ; Spanish public funds[ESP2017-87676-2-2] ; Spanish public funds[ESP2017-87676-C5-5-R] ; 'Ramon y Cajal' program of the Spanish Ministry of Science and Education[RYC2012-09913] ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme[670519: MAMSIE] ; KULeuven Research Council[C16/18/005: PARADISE] ; Research Foundation Flanders (FWO)[G0H5416N] ; BELgian federal Science Policy Office (BELSPO) through PRODEX grant PLATO ; Spanish State Research Agency (AEI)[ESP2017-87676-C5-1-R] ; Spanish State Research Agency (AEI)[MDM-2017-0737] ; National Research, Development and Innovation Fund of Hungary[PD-123910] ; National Research, Development and Innovation Fund of Hungary[PD1717] ; Whitaker Foundation ; Natural Sciences and Engineering Research Council of Canada ; 'Programme National de Physique Stellaire' (PNPS) of CNRS/INSU - CEA ; CNES ; Polish NCN[2015/18/A/ST9/00578] ; Postdoc@MUNI project[CZ.02.2.69/0.0/0.0/16-027/0008360] ; State Agency for Research of the Spanish MCIU through the 'Center of Excellence Severo Ochoa' award[SEV-2017-0709] ; STFC[ST/N504348/1] ; STFC[ST/R000603/1] ; DGAPA-UNAM[PAPIIT IN100918] ; Ministry of Science and Technology of Thailand ; French Agence Nationale de la Recherche (ANR), under grant ESRR[ANR-16-CE31-0007-01] ; NSFC of China[11873084] ; NSFC of China[11521303] ; YunnanApplied Basic Research Projects[2017B008] ; Bulgarian NSF[DN 08-1/2016] ; Fonds Wetenschappelijk Onderzoek - Vlaanderen (FWO)[G0H5416N] ; National Aeronautics and Space Administration ; National Science Foundation ; [DN 18/13-12.12.2017]
项目资助者NASA Explorer Program ; Danish National Re-search Foundation[DNRF106] ; ESA PRODEX[PEA 4000119301] ; Stellar Astrophysics Centre (SAC) at Aarhus University ; NASA[NAS5-2655] ; Danish National Research Foundation[DNRF106] ; FCT -Fundacao para a Ciencia e a Tecnologia ; FEDER through COMPETE2020 -Programa Operacional Competitividade e Internacionalizacao[UID/FIS/04434/2019, PTDC/FIS-AST/30389/2017, POCI-01-0145-FEDER-030389] ; FCT[CEECIND/02619/2017] ; Polish National Science Center (NCN)[2018/29/B/ST9/02803] ; Polish National Science Center (NCN)[2015/18/A/ST9/00578, 2016/21/B/ST9/01126] ; Spanish public funds under Spanish Ministry of Science and Education[ESP201787676-2-2, ESP2015-65712-C5-5-R] ; NSF REU program[PHY-1359195] ; Lendulet Program of the Hungarian Academy of Sciences[LP2018-7/2018] ; National Research, Development and Innovation Fund of Hungary under the K16 funding scheme[115709] ; Spanish public funds[ESP2015-65712-C5-5-R, ESP2017-87676-2-2, ESP2017-87676-C5-5-R] ; 'Ramon y Cajal' program of the Spanish Ministry of Science and Education[RYC2012-09913] ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme[670519: MAMSIE] ; KULeuven Research Council[C16/18/005: PARADISE] ; Research Foundation Flanders (FWO)[G0H5416N] ; BELgian federal Science Policy Office (BELSPO) through PRODEX grant PLATO ; Spanish State Research Agency (AEI)[ESP2017-87676-C5-1-R, MDM-2017-0737] ; National Research, Development and Innovation Fund of Hungary[PD-123910, PD1717] ; Whitaker Foundation ; Natural Sciences and Engineering Research Council of Canada ; 'Programme National de Physique Stellaire' (PNPS) of CNRS/INSU - CEA ; CNES ; Polish NCN[2015/18/A/ST9/00578] ; Postdoc@MUNI project[CZ.02.2.69/0.0/0.0/16-027/0008360] ; State Agency for Research of the Spanish MCIU through the 'Center of Excellence Severo Ochoa' award[SEV-2017-0709] ; STFC[ST/N504348/1, ST/R000603/1] ; DGAPA-UNAM[PAPIIT IN100918] ; Ministry of Science and Technology of Thailand ; French Agence Nationale de la Recherche (ANR), under grant ESRR[ANR-16-CE31-0007-01] ; NSFC of China[11873084, 11521303] ; YunnanApplied Basic Research Projects[2017B008] ; Bulgarian NSF[DN 08-1/2016] ; Fonds Wetenschappelijk Onderzoek - Vlaanderen (FWO)[G0H5416N] ; National Aeronautics and Space Administration ; National Science Foundation ; [DN 18/13-12.12.2017]
语种英语
学科领域天文学 ; 恒星与银河系 ; 恒星天文学
文章类型Article
出版者OXFORD UNIV PRESS
出版地GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
ISSN0035-8711
URL查看原文
归档日期https://academic.oup.com/mnras/article/490/3/4040/5583021
WOS记录号WOS:000503993100070
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]PERIOD-LUMINOSITY RELATION ; LINE-PROFILE VARIATIONS ; MAIN-SEQUENCE STARS ; MAGNETIC AP STARS ; TO-CORE ROTATION ; PULSATIONAL INSTABILITY ; CHEMICAL-COMPOSITION ; METALLIC-LINE ; ASTEROSEISMIC MEASUREMENT ; COMBINATION FREQUENCIES
EI入藏号20221712024328
EI主题词Stars
EI分类号657.2 Extraterrestrial Physics and Stellar Phenomena
引用统计
被引频次:87[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/22030
专题恒星物理研究组
中国科学院天体结构与演化重点实验室
通讯作者Antoci, V.
作者单位1.Stellar Astrophysics Centre, Ny Munkegade 120, D-8000 Aarhus, Denmark
2.Instituto de Astrof´ısica e Ciencias do Espac ˆ ¸o, Universidade do Porto, CAUP, Rua das Estrelas, P-4150-762 Porto, Portugal
3.Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium
4.Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia
5.Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK
6.LESIA, Observatoire de Paris, Universite PSL, CNRS, Sorbonne Univer- ´ site, Universit ´ e de Paris, 5 place Jules Janssen, F-92195 Meudon, France
7.Instytut Astronomiczny, Uniwersytet Wrocławski, Kopernika 11, PL-51-622 Wrocław, Poland
8.Instituto de Astronom´ıa, Universidad Nacional Autonoma de M ´ exico, Ap. ´ P. 877, Ensenada, BC 22860, Mexico
9.Departamento F´ısica Teorica y del Cosmos, Universidad de Granada, ´ Campus de Fuentenueva s/n, E-18071 Granada, Spain
10.Instituto de Astrof´ısica de Andaluc´ıa (CSIC), Glorieta de la Astronom´ıa s/n, E-18008 Granada, Spain
11.Department of Physics, Institute for Advanced Studies in Basic Sciences (IASBS), Zanjan 45137-66731, Iran
12.Department of Physics, Faculty of Science, University of Zanjan, P.O. Box 45195-313 Zanjan, Iran
13.Nicolaus Copernicus Astronomical Center, Bartycka 18, PL-00-716 Warsaw, Poland
14.Physics Department, Faculty of Sciences and Arts, C¸ anakkale Onsekiz Mart University, 17100 C¸ anakkale, Turkey
15.Center for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA
16.Department of Physics and Astronomy, University of British Columbia, Vancouver, Canada
17.Department of Theoretical Physics and Astrophysics, Masaryk University, Kotlarska 2, CZ-611 37 Brno, Czech Republic
18.Instituto de Astrof´ısica La Plata, CONICET-UNLP, Paseo del Bosque s/n, 1900 La Plata, Argentina
19.Department of Physics, Lehigh University, 16 Memorial Drive East, Bethlehem, PA 18015, USA
20.School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85281, USA
21.Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
22.Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
23.Department of Aeronautics and Astronautics, MIT, 77 Massachusetts Avenue, Cambridge, MA 02139, USA
24.Astrophysics Group, Keele University, Staffordshire ST5 5BG, UK
25.Department of Physics, University of York, Heslington, York YO10 5DD, UK
26.Konkoly Observatory, CSFK, Konkoly Thege Miklos´ ut 15-17, H-1121 ´ Budapest, Hungary
27.22 MTA CSFK Lendulet Near-Field Cosmology Research Group
28.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, P.R. China
29.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, P.R. China
30.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, P.R. China
31.Chinese Acad Sci, Ctr Astron Mega Sci, 20A Datun Rd, Beijing 100012, Peoples R China
32.Departamento de Astrof´ısica, Centro de Astrobiolog´ıa (CSIC-INTA), ESAC, Camino Bajo del Castillo s/n, E-28692 Madrid, Spain
33.Department of Chemistry and Physics, Florida Gulf Coast University, 10501 FGCU Blvd., Fort Myers, FL 33965, USA
34.Royal Observatory of Belgium, Ringlaan 3, B-1180 Brussel, Belgium
35.Center for Exoplanets and Habitable Worlds, 525 Davey Laboratory, The Pennsylvania State University, University Park, PA 16802, USA
36.Los Alamos National Laboratory, MS T-082, Los Alamos, NM 87545, USA
37.Physics Department, Bloomsburg University, 200 E 2nd St, Bloomsburg, PA 17815, USA
38.Physics Department, Mount Allison University, Sackville, NB E4L 1E6, Canada
39.Astrophysics Research Group, Faculty of Engineering and Physical Sciences, University of Surrey, Guildford GU2 7XH, UK
40.National Astronomical Research Institue of Thailand, 260 Moo 4, T. Donkaew, A. Maerim, Chiangmai 50180, Thailand
41.Departamento de F´ısica e Astronomia, Faculdade de Ciencias da Univer- ˆ sidade do Porto, Porto, Portugal
42.Department of Physics & Astronomy, Camosun College, Victoria, BC, Canada
43.IRAP, Universite de Toulouse, CNRS, UPS, CNES, 14 Avenue Edouard ´ Belin, F-31400 Toulouse, France
44.Department of Theoretical Physics and Astrophysics, Masaryk University, Kotla´rsk ˇ a 2, CZ-61137 Brno, Czech Republic
45.Astronomical Institute, Czech Academy of Sciences, Fricova 298, CZ- ˇ 25165 Ondrejov, Czech Republic
46.Institute of Astronomy and NAO, Bulgarian Academy of Sciences, Blvd.Tsarigradsko Chaussee 72, Sofia 1784, Bulgaria
47.Institute for Astrophysics, University of Vienna, Turkenschanzstrasse 17, ¨ A-1180 Vienna, Austria
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Antoci, V.,Cunha, M. S.,Bowman, D. M.,et al. The first view of delta Scuti and gamma Doradus stars with the TESS mission[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2019,490(3):4040-4059.
APA Antoci, V..,Cunha, M. S..,Bowman, D. M..,Murphy, S. J..,Kurtz, D. W..,...&Weiss, W. W..(2019).The first view of delta Scuti and gamma Doradus stars with the TESS mission.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,490(3),4040-4059.
MLA Antoci, V.,et al."The first view of delta Scuti and gamma Doradus stars with the TESS mission".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 490.3(2019):4040-4059.
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