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相关论文: KIC 3858884: a hybrid {\delta} Sct pulsator in a h…

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We present Kepler satellite photometry of KIC 10661783, a short-period binary star system which shows total eclipses and multi-periodic delta Scuti pulsations. A frequency analysis of the eclipse-subtracted light curve reveals at least 68…

KIC~8262223 is an eclipsing binary with a short orbital period ($P=1.61$ d). The {\it Kepler} light curves are of Algol-type and display deep and partial eclipses, ellipsoidal variations, and pulsations of Delta Scuti type. We analyzed the…

太阳与恒星天体物理 · 物理学 2017-03-15 Zhao Guo , Douglas R. Gies , Rachel A. Matson , Antonio García Hernández , Zhanwen Han , Xuefei Chen

Context: Several hundred candidate hybrid pulsators of type A-F have been identified from space-based observations. Their large number allows both statistical analyses and detailed investigations of individual stars. This offers the…

We present the results of analysis and modelling of the eclipsing binary system, KIC 10661783. The Fourier analysis of the Kepler light curve, corrected for the binary effects, reveals 750 frequency peaks in both p and g-mode regions. Those…

太阳与恒星天体物理 · 物理学 2020-02-03 Amadeusz Miszuda , Wojciech Szewczuk , Jadwiga Daszyńska-Daszkiewicz

We carried out light curve solutions of two eclipsing detached binaries on eccentric orbits observed by Kepler. The orbits and fundamental parameters of KIC 11619964 and KIC 7118545 were determined with a high accuracy by modeling of their…

太阳与恒星天体物理 · 物理学 2015-07-23 Diana Kjurkchieva , Doroteya Vasileva

We carried out light curve solutions of ten detached eclipsing eccentric binaries observed by Kepler. The formal errors of the derived parameters from the light curve solutions are below 1%. Our results give indications that the components…

太阳与恒星天体物理 · 物理学 2016-05-25 D. Kjurkchieva , D. Vasileva

Stellar theory enables us to understand the properties of stars at different stages of their evolution, and contributes to other fields of astrophysics such as galactic and exoplanet studies. Assessing the accuracy of stellar theories…

太阳与恒星天体物理 · 物理学 2024-08-07 Z. Jennings , J. Southworth , S. A. Rappaport , T. Borkovits , G. Handler , D. W. Kurtz

Theories of stellar convective core overshoot can be examined through analysis of pulsating stars. Better accuracy can be achieved by obtaining external constraints such as those provided by observing pulsating stars in eclipsing binary…

太阳与恒星天体物理 · 物理学 2022-02-16 Padraic Odesse , Catherine Lovekin

Eclipsing binary systems with components that pulsate in gravity modes ($g$ modes) allow for simultaneous and independent constraints of the chemical mixing profiles of stars. We aim to assemble a sample of $g$-mode pulsators in detached…

太阳与恒星天体物理 · 物理学 2020-11-25 S. Sekaran , A. Tkachenko , M. Abdul-Masih , A. Prsa , C. Johnston , D. Huber , S. J. Murphy , G. Banyard , A. W. Howard , H. Isaacson , D. M. Bowman , C. Aerts

The present paper focuses on the eclipsing binary KIC 8553788 which belongs to two different types of binary systems regarding its physical properties. In particular, it is one of the 71 oscillating stars of Algol type that have been…

太阳与恒星天体物理 · 物理学 2018-09-05 Alexios Liakos

The eccentricity, periastron angle, orbital inclination, mass ratio, stellar temperatures and relative stellar radii of 12 eclipsing eccentric binaries were determined on the basis of Kepler data. The analysis of their out-of-eclipse…

太阳与恒星天体物理 · 物理学 2016-12-28 Diana Kjurkchieva , Doroteya Vasileva , Dinko Dimitrov

Context. This research paper contains light curve modelling, spectroscopy and detailed asteroseismic studies for four out of five in total semidetached eclipsing binaries with a delta Scuti component, that have been detected to date through…

太阳与恒星天体物理 · 物理学 2017-11-22 Alexios Liakos

The present work concerns the Asteroseismology of the Kepler detached eclipsing binary KIC 8504570. Particularly, it focuses on the pulsational behaviour of the oscillating component of this system and the estimation of its physical…

太阳与恒星天体物理 · 物理学 2020-10-21 Alexios Liakos , Panagiotis Niarchos

KIC 8569819 is an eclipsing binary star with an early F primary and G secondary in a 20.85-d eccentric orbit. The primary is a delta Sct - gamma Dor star pulsating in both p modes and g modes. Using 4 years of Kepler Mission photometric…

太阳与恒星天体物理 · 物理学 2015-06-23 Donald W. Kurtz , Kelly M. Hambleton , Hiromoto Shibahashi , Simon J. Murphy , Andrej Prsa

We determined the orbits and stellar parameters of three eccentric eclipsing binaries by light curve solutions of their Kepler data. KIC 10992733 and KIC 5632781 undergo total eclipses while KIC 10026136 reveals partial eclipses. The…

太阳与恒星天体物理 · 物理学 2017-07-26 Diana Kjurkchieva , Doroteya Vasileva

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

We determined the orbits and stellar parameters of three eccentric eclipsing binaries by light curve solutions of their Kepler data. KIC 8111622 and KIC 10518735 undergo total eclipses while KIC 8196180 reveals partial eclipses. The target…

太阳与恒星天体物理 · 物理学 2018-01-31 Diana P. Kjurkchieva , Doroteya L. Vasileva

We present both binarity and pulsation of KIC 6220497 from the {\it Kepler} observations. The light curve synthesis shows that the eclipsing system is a semi-detached Algol with parameters of $q$ = 0.243$\pm$0.001, $i$ = 77.3$\pm$0.3 deg,…

太阳与恒星天体物理 · 物理学 2016-06-15 Jae Woo Lee , Kyeongsoo Hong , Seung-Lee Kim , Jae-Rim Koo

We report spectroscopic observations for 19 $\delta$\,Sct candidates observed by the {\it Kepler} satellite both in long and short cadence mode. For all these stars, by using spectral synthesis, we derive the effective temperature, the…

{KIC~8975515 is a \emph{Kepler} double-lined spectroscopic binary system with hybrid pulsations. Two components have similar atmospheric properties (T$_{\rm eff}$ $\sim$ 7400~K), and one of them is a fast rotator ($v\sin i = 162$ versus 32…

太阳与恒星天体物理 · 物理学 2020-07-01 A. Samadi-Ghadim , P. Lampens , D. M. Jassur , P. Jofré