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相关论文: Chromospherically Active Low-Mass Close Binary: KI…

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We present a detailed study of the two Sun-like stars KIC 7985370 and KIC 7765135, aimed at determining their activity level, spot distribution, and differential rotation. Both stars were discovered by us to be young stars and were observed…

太阳与恒星天体物理 · 物理学 2015-06-05 H. -E. Fröhlich , A. Frasca , G. Catanzaro , A. Bonanno , E. Corsaro , J. Molenda-Żakowicz , A. Klutsch , D. Montes

We present photodynamical models of four eclipsing binary systems that are members of higher-order multiple systems. We provide some radial velocities measurements and use recent TESS data for three of the systems. KIC 7668648 consists of…

太阳与恒星天体物理 · 物理学 2023-12-12 Jerome A. Orosz

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

The eclipsing binary T-Cyg1-12664 was observed both spectroscopically and photometrically. Radial velocities of both components and ground-based VRI light curves were obtained. The Kepler's R-data and radial velocities for the system were…

太阳与恒星天体物理 · 物理学 2015-06-11 O. Cakirli , C. Ibanoglu , E. Sipahi

The unparalleled photometric data obtained by NASA's Kepler Space Telescope has led to an improved understanding of stellar structure and evolution - in particular for solar-like oscillators in this context. Binary stars are fascinating…

We present spectroscopic and photometric analysis of the eclipsing binary KIC\,7385478. We find that the system is formed by F1V + K4III-IV components. Combining results from analysis of spectroscopic data and $Kepler$ photometry, we…

太阳与恒星天体物理 · 物理学 2017-08-23 Orkun Özdarcan , Hasan Ali Dal

We present the eclipsing Heartbeat Star KIC 9704906 with tidally excited oscillations (TEOs) and gamma Doradus/delta Scuti hybrid pulsations. The derived parameters show that it has an orbital period of $P$=8.7529108(1) days, a high…

太阳与恒星天体物理 · 物理学 2024-12-10 Min-Yu Li , Sheng-Bang Qian , Li-Ying Zhu , Liang Liu , Wen-Ping Liao , Er-Gang Zhao , Xiang-Dong Shi , Fu-Xing Li , Qi-Bin Sun

We analyzed a Kepler light curve of KIC 8751494, a recently recognized novalike cataclysmic variable in the Kepler field. We detected a stable periodicity of 0.114379(1) d, which we identified as being the binary's orbital period. The…

太阳与恒星天体物理 · 物理学 2015-06-15 Taichi Kato , Hiroyuki Maehara

We present results regarding the longitudinal migrations of cool stellar spots that exhibit remarkable oscillations and explore their possible causes. We conducted analyses using high-quality data from nine target systems of various…

太阳与恒星天体物理 · 物理学 2024-04-15 N. Ö. Kaya , H. A. Dal

The first multi-color light curve analysis of the AH Mic binary system is presented. This system has very few past observations from the southern hemisphere. We extracted the minima times from the light curves based on the Markov Chain…

We investigated the pulsating behavior of KIC 10855535 using Kepler 4-year long cadence data. Two independent frequencies were detected: a pulsation frequency F0 = 17.733260(5)d-1 and a low frequency f8=0.412643(8)d-1 We identify F0 as the…

太阳与恒星天体物理 · 物理学 2024-11-05 Lixian Shen , Ali Esamdin , Chenglong Lv , Haozhi Wang , Taozhi Yang , Rivkat Karimov , Shuhrat A. Ehgamberdiev , Hubiao Niu , Jinzhong Liu

We present a photometric, spectroscopic, asteroseismic, and evolutionary analysis of the Algol-type eclipsing binary KIC 12268220. We find the O'Connell effect and anticorrelated eclipse timing variations in the Kepler light curve,…

太阳与恒星天体物理 · 物理学 2020-08-12 Kaiming Cui , Zhao Guo , Qing Gao , Juanjuan Ren , Junbo Zhang , Yutao Zhou , Jifeng Liu

HD 81809 has one of the highest quality activity cycles from the sample of stars synoptically observed in the Mount Wilson Observatory HK Project. However, this object is in fact a binary system, raising the question as to which of the…

太阳与恒星天体物理 · 物理学 2018-10-24 Ricky Egeland

Reanalyzing contact binaries with space-based photometric data and investigating possible parameter changes can yield accurate samples for theoretical studies. We investigated light curve solutions and fundamental parameters for twenty…

太阳与恒星天体物理 · 物理学 2024-05-30 Ehsan Paki , Atila Poro

We present a comprehensive study of the eclipsing binary system KIC 10661783. The analysis of the whole Kepler light curve, corrected for the binary effects, reveals a rich oscillation spectrum with 590 significant frequency peaks, 207 of…

太阳与恒星天体物理 · 物理学 2021-06-08 A. Miszuda , W. Szewczuk , J. Daszyńska-Daszkiewicz

In the faint star KIC 9700322 observed by the Kepler satellite, 76 frequencies with amplitudes from 14 to 29000 ppm were detected. The two dominant frequencies at 9.79 and 12.57 c/d (113.3 and 145.5 \mu Hz), interpreted to be radial modes,…

Effective temperatures, surface gravities, and iron abundances were derived for 109 stars observed by the K2 mission using equivalent width measurements of Fe I and Fe II lines. Calculations were carried out in LTE using Kurucz model…

太阳与恒星天体物理 · 物理学 2024-07-19 V. Loaiza-Tacuri , Katia Cunha , Verne V. Smith , F. Quispe-Huaynasi , Ellen Costa-Almeida , Luan Ghezzi , Jorge Melendez

In this study, investigation of two double-lined binary stars KIC 5113146 and KIC 5111815 in NGC 6819 is presented based on both photometric and spectroscopic data. Simultaneous analysis of light and radial velocity curves was made and the…

太阳与恒星天体物理 · 物理学 2022-07-27 E. Soydugan , F. Alicavus , F. Soydugan , S. Bilir

Neuhaeuser & Comeron (1998, 1999) presented direct imaging evidence, as well as first spectra, of several young stellar and sub-stellar M6- to M8-type objects in the Cha I dark cloud. One of these objects is Cha Halpha 2, classified as…

天体物理学 · 物理学 2009-11-13 T. O. B. Schmidt , R. Neuhäuser , N. Vogt , A. Seifahrt , T. Roell , A. Bedalov

The light curves of solar-type stars present both periodic fluctuation and flare spikes. The gradual periodic fluctuation is interpreted as the rotational modulation of magnetic features on the stellar surface and is used to deduce magnetic…

太阳与恒星天体物理 · 物理学 2018-05-15 Han He , Huaning Wang , Mei Zhang , Ahmad Mehrabi , Yan Yan , Duo Yun