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相关论文: CCD Photometry of Delta Scuti stars 7 Aql and 8 Aq…

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We report a multisite photometric campaign for the Beta Cephei star 12 Lacertae. 750 hours of high-quality differential photoelectric Stromgren, Johnson and Geneva time-series photometry were obtained with 9 telescopes during 190 nights.…

The Praesepe cluster contains a number of Delta Sct and Gamma Dor pulsators. Asteroseismology of cluster stars is simplified by the common distance, age and stellar abundances. Since asteroseismology requires a large number of known…

Period analysis of CCD photometry of V1493 Aql (Nova Aql 1999 no. 1) performed during 12 nights through I and R filters a few weeks after maximum is presented. The PDM method for period analysis (Stellingwerf 1978) is used. The photometric…

天体物理学 · 物理学 2009-11-11 Andrej Dobrotka , Michael Friedjung , Alon Retter , Ladislav Hric , Rudolf Novak

In Delta Scuti star models, the calculated amplitude ratios and phase differences for multi-colour photometry exhibit a strong dependence on convection. These observables are tools for determination of the spherical harmonic degree of the…

天体物理学 · 物理学 2009-11-07 J. Daszynska-Daszkiewicz , W. A. Dziembowski , A. A. Pamyatnykh

The search for chemically peculiar (CP) stars in open clusters using photoelectric photometry sampling the presence of the characteristic flux depression feature at 5200A via the Delta a-system (Maitzen 1976) has so far delivered data for…

天体物理学 · 物理学 2007-05-23 H. M. Maitzen , M. Rode , E. Paunzen

High-resolution spectroscopic observations of the rapidly rotating delta Scuti star gamma Bootis have been carried out on 2005, over 6 consecutive nights, in order to search for line-profile variability. Time series, consisting of flux…

天体物理学 · 物理学 2009-11-13 R. Ventura , G. Catanzaro , J. Christensen-Dalsgaard , M. P. Di Mauro , L. Paterno'

The evolutionary stage of the delta Scuti star 44 Tau has been unclear. Recent asteroseismic studies have claimed models on the main sequence, as well as in the expansion phase of the post-main sequence evolution. However, these models…

太阳与恒星天体物理 · 物理学 2015-05-14 P. Lenz , A. A. Pamyatnykh , T. Zdravkov , M. Breger

We have explored a sample of suspected A-type binaries in a systematic way, both spectroscopically and photometrically. Due to their location in the H-R diagram, indications of pulsation and/or chemical peculiarities among these suspected…

Statistical analyses of several Delta Scuti stars (FG Vir, 44 Tau, BL Cam and others) show that the photometrically observed frequencies cluster around the frequencies of the radial modes over many radial orders. The observed regularities…

天体物理学 · 物理学 2008-11-03 M. Breger , P. Lenz , A. A. Pamyatnykh

We have searched for photometric variability in 95 Vir, a fast rotating, chromospherically active early F-type star, which was observed in the framework of Campaign 6 of the Kepler K2 mission. Available literature information on 95 Vir were…

太阳与恒星天体物理 · 物理学 2017-04-19 Ernst Paunzen , Stefan Huemmerich , Klaus Bernhard , Przemek Walczak

We present and discuss the pulsational characteristics of the Delta Scuti star 38 Eri from photometric data obtained at two widely spaced epochs, partly from the ground (1998) and partly from space (MOST, 2011). We found 18 frequencies…

A comparison between linear stability analysis and observations of pulsation modes in five delta Scuti stars, belonging to the same cluster, is presented. The study is based on the work by Michel et al. (1999), in which such a comparison…

天体物理学 · 物理学 2009-06-23 J. C. Suarez , E. Michel , G. Houdek , F. Perez Hernandez , Y. Lebreton

Several Delta Sct stars were photometrically monitored with the satellite CoRoT and observed in high-resolution spectroscopy from ground. We present here the preliminary analysis of the abundance analysis of several potential CoRoT targets.…

太阳与恒星天体物理 · 物理学 2015-05-19 E. Poretti , L. Mantegazza , E. Niemczura , M. Rainer , T. Semaan , T. Luftinger , A. Baglin , M. Auvergne , E. Michel , R. Samadi

We describe the search for delta Scuti stars in the MACHO database of bulge fields. Concentrating on a sample of high amplitude delta Scutis, we examine the light curves and pulsation modes. We also discuss their spatial distribution and…

Thanks to relatively firm mode identification, possible based on period ratios only, High Amplitude Delta Scuti Stars pulsating in at least three radial modes are promising targets for asteroseismic inference. In this study we used the most…

太阳与恒星天体物理 · 物理学 2022-07-20 H. Netzel , R. Smolec

While delta Scuti stars are the most numerous class of kappa-mechanism pulsators in the instability strip, the short periods and small peak-to-peak amplitudes have left them understudied and underutilized. Recently, large-scale time-domain…

We present a mode identification based on new high-resolution time-series spectra of the non-radially pulsating Delta Scuti star FG~Vir (HD 106384, V = 6.57, A5V). From 2002 February to June a global Delta Scuti Network (DSN) campaign,…

In this work, the pulsation analysis is performed on 83 high-amplitude $\delta$ Scuti stars, which have been observed by the Transiting Exoplanet Survey Satellite (TESS). The results show that 49 of these HADS show single-mode pulsation, 27…

太阳与恒星天体物理 · 物理学 2023-07-10 Wangjunting Xue , Jia-Shu Niu , Hui-Fang Xue , Sijing Yin

We perform mode identification for five $\delta$ Scuti stars in the Pleiades star cluster, using custom light curves from K2 photometry. By creating \'echelle diagrams, we identify radial and dipole mode ridges, comprising a total of 28…

太阳与恒星天体物理 · 物理学 2022-02-09 Simon J. Murphy , Timothy R. Bedding , Timothy R. White , Yaguang Li , Daniel Hey , Daniel Reese , Meridith Joyce

We review the current status of different mode-identification techniques based on observed line-profile variations. Three basic methods are currently available to identify the non-radial pulsation modes. These three methods are described,…

天体物理学 · 物理学 2007-05-23 Conny Aerts , Laurent Eyer