2019
The first view of delta Scuti and gamma Doradus stars with the TESS mission
ANTOCI, V., M.S. CUNHA, D.M. BOWMAN, S.J. MURPHY, D.W. KURTZ et. al.Základní údaje
Originální název
The first view of delta Scuti and gamma Doradus stars with the TESS mission
Autoři
ANTOCI, V., M.S. CUNHA, D.M. BOWMAN, S.J. MURPHY, D.W. KURTZ, T.R. BEDDING, C.C. BORRE, S. CHRISTOPHE, J. DASZYNSKA-DASZKIEWICZ, L. FOX-MACHADO, A.G. HERNANDEZ, H. GHASEMI, R. HANDBERG, H. HANSEN, A. HASANZADEH, G. HOUDEK, C. JOHNSTON, A.B. JUSTESEN, F.K. ALICAVUS, K. KOTYSZ, D. LATHAM, J.M. MATTHEWS, J. MONSTER, E. NIEMCZURA, Ernst PAUNZEN (40 Rakousko, domácí), J.P.S. ARIAS, A. PIGULSKI, J. PEPPER, T. RICHEY-YOWELL, H. SAFARI, S. SEAGER, B. SMALLEY, T. SHUTT, A. SODOR, J.C. SUAREZ, A. TKACHENKO, T. WU, K. ZWINTZ, S.B. FORTEZA, E. BRUNSDEN, Z. BOGNAR, D.L. BUZASI, S. CHOWDHURY, Cat P. DE, J.A. EVANS, Z. GUO, J.A. GUZIK, N. JEVTIC, P. LAMPENS, M.L. MARTIZ, C. LOVEKIN, G. LI, G.M. MIROUH, D. MKRTICHIAN, M. J. P. F. G. MONTEIRO, J.M. NEMEC, R.M. OUAZZANI, J. PASCUAL-GRANADO, D.R. REESE, M. RIEUTORD, J.R. RODON, Marek SKARKA (203 Česká republika, domácí), P. SOWICKA, I. STATEVA, R. SZABO a W.W. WEISS
Vydání
Monthly Notices of the Royal Astronomical Society, MALDEN, WILEY, 2019, 0035-8711
Další údaje
Jazyk
angličtina
Typ výsledku
Článek v odborném periodiku
Obor
10308 Astronomy
Stát vydavatele
Velká Británie a Severní Irsko
Utajení
není předmětem státního či obchodního tajemství
Odkazy
Impakt faktor
Impact factor: 5.357
Kód RIV
RIV/00216224:14310/19:00113426
Organizační jednotka
Přírodovědecká fakulta
UT WoS
000503993100070
Klíčová slova anglicky
asteroseismology; techniques: photometric; stars: chemically peculiar; stars: interiors; stars: variables: delta Scuti
Štítky
Příznaky
Mezinárodní význam, Recenzováno
Změněno: 31. 3. 2020 21:01, Mgr. Marie Šípková, DiS.
Anotace
V originále
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.
Návaznosti
EF16_027/0008360, projekt VaV |
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