The first view of delta Scuti and gamma Doradus stars with the TESS mission
文献类型:期刊论文
作者 | 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 |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
出版日期 | 2019-12-01 |
卷号 | 490期号:3页码:4040-4059 |
ISSN号 | 0035-8711 |
关键词 | asteroseismology techniques: photometric stars: chemically peculiar stars: interiors stars: variables: delta Scuti |
DOI | 10.1093/mnras/stz2787 |
产权排序 | 第28完成单位 |
文献子类 | Article |
英文摘要 | 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. |
学科主题 | 天文学 ; 恒星与银河系 ; 恒星天文学 |
URL标识 | 查看原文 |
出版地 | GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND |
WOS关键词 | 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 |
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] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | OXFORD UNIV PRESS |
WOS记录号 | WOS:000503993100070 |
资助机构 | 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] |
源URL | [http://ir.ynao.ac.cn/handle/114a53/22029] |
专题 | 云南天文台_恒星物理研究组 云南天文台_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 |
推荐引用方式 GB/T 7714 | 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. |
入库方式: OAI收割
来源:云南天文台
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