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相关论文: Hybrid gamma Doradus/delta Scuti Stars: Comparison…

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Observations from space missions have allowed significant progress in many scientific domains due to the absence of atmospheric noise contributions and having uninterrupted data sets. In the context of asteroseismology, this has been…

太阳与恒星天体物理 · 物理学 2023-08-16 Julieta Sánchez Arias , Orlagh Louise Creevey , Eric Chapellier , Bernard Pichon

In this work we propose a preliminary seismic investigation of $\delta$ Scuti stars in the Pleiades cluster, focusing on potential diagnostics of convection and core-overshooting. Taking into account the effect of fast rotation in the…

天体物理学 · 物理学 2007-05-23 J. C. Suarez , E. Michel , G. Houdek , Y. Lebreton , F. Perez Hernandez

Ground-based spectroscopic follow-up observations of the pulsating stars observed by the Kepler satellite mission are needed for their asteroseismic modelling. We aim to derive the fundamental parameters for a sample of 26 Gamma Doradus…

太阳与恒星天体物理 · 物理学 2015-06-04 Andrew Tkachenko , Holger Lehmann , Barry Smalley , Jonas Debosscher , Conny Aerts

Based on the LAMOST spectroscopy and TESS time-series photometry, we have obtained a main-sequence star sample of $\delta$ Scuti and $\gamma$ Doradus stars. The sample includes 1534 $\delta$ Sct stars, 367 $\gamma$ Dor stars, 1703 $\delta$…

太阳与恒星天体物理 · 物理学 2024-11-15 Jiyu Wang , Xiaodian Chen , Licai Deng , Jianxing Zhang , Weijia Sun

Intermediate mass Pre-main sequence stars (1.5 $M_{\odot}< M < 5M_{\odot}$) cross the instability strip on their way to the main sequence. They are therefore expected to be pulsating in a similar way as the $\delta$ Scuti stars. In this…

天体物理学 · 物理学 2010-12-09 V. Ripepi , M. Marconi , F. Palla , S. Bernabei , A. Ruoppo , F. Cusano , J. M. Alcala'

Pulsating subdwarf B stars oscillate in short-period $p$-modes or long-period $g$-modes. HS 0702 + 6043 is one of currently three objects known to show characteristics of both types and hence is classified as hybrid pulsator. We briefly…

天体物理学 · 物理学 2008-12-31 R. Lutz , S. Schuh , R. Silvotti , R. Kruspe , S. Dreizler

$\gamma$ Doradus stars are photometrically variable early F-type stars on or just above the main sequence in the Hertzsprung-Russell Diagram. They vary by as much as 0.1 mag on time scales an order of magnitude slower than the fundamental…

天体物理学 · 物理学 2015-06-24 Kevin Krisciunas , Richard A. Crowe , Kenneth D. Luedeke , Mavourneen Roberts

We present results of a spectroscopic study of 37 southern (candidate) gamma Doradus stars based on echelle spectra. The observed spectra were cross-correlated with the standard template spectrum of an F0-type star for an easier detection…

GK Dra is a detached eclipsing binary system containing two early-F stars, one evolved, in an orbit with a period of 9.974 d and a small eccentricity. Its eclipsing nature was discovered using Hipparcos data, and pulsations were found in…

太阳与恒星天体物理 · 物理学 2024-01-25 John Southworth

The MONS space experiment will be able to verify some of the most important topics in the asteroseismologic studies of Delta Sct and Gamma Dor stars. We discuss how the $\gamma$ Doradus can be considered possible "bridges" between the…

天体物理学 · 物理学 2007-05-23 F. M. Zerbi , E. Poretti , C. Aerts , G. Handler , A. B. Kaye

A photometric variability study of a sample of northern field stars, which previously classified as either PMS or Herbig Ae/Be objects, has been undertaken with the purpose of detecting {\delta} Scuti-type pulsations. Determination of…

太阳与恒星天体物理 · 物理学 2014-09-05 D. Díaz-Fraile , E. Rodríguez , P. J. Amado

As part of the NASA Kepler Guest Observer program, we requested and obtained long-cadence data on about 2700 faint (magnitude 14-16) Kepler stars with effective temperatures and surface gravities that lie near or within the pulsation…

太阳与恒星天体物理 · 物理学 2014-04-01 Joyce A. Guzik , P. A. Bradley , J. Jackiewicz , K. Uytterhoeven , K. Kinemuchi

In this study, pulsational and physical characteristics of two $\delta$ Scuti stars, V775 Tau and V483 Tau, are analysed by using four-year high-precision photometric data of STEREO satellite. Thus, it is aimed to gain new insights into…

太阳与恒星天体物理 · 物理学 2018-09-05 Dogus Ozuyar

We present the characterization of KIC 4142768, an eclipsing binary with two evolved A-type stars in an eccentric orbit with a period of 14 days. We measure the fundamental parameters of the two components ($M_1=2.05M_{\odot},…

太阳与恒星天体物理 · 物理学 2020-01-08 Zhao Guo , Jim Fuller , Avi Shporer , Gang Li , Kelly Hambleton , Joseph Manuel , Simon Murphy , Howard Isaacson

Gamma Doradus stars present an incredibly rich pulsation spectra, with gravito-inertial modes, in some cases supplemented with delta Scuti-like pressure modes and in numerous cases with Rossby modes. The present paper aims at showing that,…

太阳与恒星天体物理 · 物理学 2020-08-12 R-M. Ouazzani , F. Lignières , M-A. Dupret , S. J. A. J. Salmon , J. Ballot , S. Christophe , M. Takata

We detect the second known lambda Bootis star (HD 54272) which exhibits gamma Doradus-type pulsations. The star was formerly misidentified as a RR Lyrae variable. The lambda Bootis stars are a small group (only 2 per cent) of late B to…

太阳与恒星天体物理 · 物理学 2015-06-19 E. Paunzen , M. Skarka , D. L. Holdsworth , B. Smalley , R. G. West

We present discoveries of the hybrid $\delta$ Scuti and $\gamma$ Doradus types stellar pulsational variability of two stars, HD 53166 and HD 53349, which were previously used as comparison in the differential photometry of a known $\delta$…

太阳与恒星天体物理 · 物理学 2023-07-25 A. -Y. Zhou

In $\gamma$ Doradus stars, the g-mode period spacing shows an approximately linear relation with period. The slope is a new asteroseismic diagnostic, related to the rotation rate and the azimuthal order $m$. We report two automated methods,…

太阳与恒星天体物理 · 物理学 2018-10-17 Gang Li , Timothy R. Bedding , Simon J. Murphy , Timothy Van Reeth , Victoria Antoci , Rhita-Maria Ouazzani

Inspection of the periodograms of TESS delta Scuti stars indicates that there is little, if any, similarity between the frequencies of stars in the same region of the H-R diagram. This is difficult to understand because pulsation models…

太阳与恒星天体物理 · 物理学 2024-01-23 Luis A. Balona