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, 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, P. SOWICKA, I. STATEVA, R. SZABO a W.W. WEISS. The first view of delta Scuti and gamma Doradus stars with the TESS mission. Monthly Notices of the Royal Astronomical Society. MALDEN: WILEY, 2019, roč. 490, č. 3, s. 4040-4059. ISSN 0035-8711. Dostupné z: https://dx.doi.org/10.1093/mnras/stz2787.
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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
Originální 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
WWW URL
Impakt faktor Impact factor: 5.357
Kód RIV RIV/00216224:14310/19:00113426
Organizační jednotka Přírodovědecká fakulta
Doi http://dx.doi.org/10.1093/mnras/stz2787
UT WoS 000503993100070
Klíčová slova anglicky asteroseismology; techniques: photometric; stars: chemically peculiar; stars: interiors; stars: variables: delta Scuti
Štítky rivok
Příznaky Mezinárodní význam, Recenzováno
Změnil Změnila: Mgr. Marie Šípková, DiS., učo 437722. Změněno: 31. 3. 2020 21:01.
Anotace
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 VaVNázev: Postdoc@MUNI
VytisknoutZobrazeno: 8. 5. 2024 10:41