J 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
Název: Postdoc@MUNI