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Related papers: Mode density and frequency extraction in the delta…

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High-amplitude $\delta$ Scuti stars (HADS) that pulsate in their first three radial modes are rare in current samples. Here, we analyse five such triple-mode HADS observed by the Transiting Exoplanet Survey Satellite (TESS) and {report that…

Solar and Stellar Astrophysics · Physics 2025-05-21 Jia-Shu Niu , Hui-Fang Xue

Harmonics are a ubiquitous feature across various pulsating stars. They are traditionally viewed as mere replicas of the independent primary pulsation modes and have thus been excluded from asteroseismological models. Recent research,…

Solar and Stellar Astrophysics · Physics 2024-07-17 Hui-Fang Xue , Jia-Shu Niu

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.…

Solar and Stellar Astrophysics · Physics 2015-05-19 E. Poretti , L. Mantegazza , E. Niemczura , M. Rainer , T. Semaan , T. Luftinger , A. Baglin , M. Auvergne , E. Michel , R. Samadi

We present our analysis of simulated data in order to derive a detection threshold which can be used in the pre-whitening process of amplitude spectra. In case of ground-based data of pulsating stars, this threshold is conventionally taken…

Solar and Stellar Astrophysics · Physics 2015-06-23 A. S. Baran , C. Koen , B. Pokrzywka

We present results of a multi-site photometric campaign on the high-amplitude $\delta$\,Scuti star KIC\,6382916 in the {\it Kepler} field. The star was observed over a 85-d interval at five different sites in North America and Europe during…

For the Delta Scuti star 44 Tau 13 independent frequencies have been detected in previous studies. This star is unusual among the Delta Scuti stars because of its very low v sin i value of 2 +/- 1 km/s, indicating that it is either an…

Astrophysics · Physics 2009-11-13 P. Lenz , A. A. Pamyatnykh , M. Breger , V. Antoci

The nature of the observed amplitude variability of several modes in the Delta Scuti star FG Vir is examined. In this star, three frequencies show strong amplitude and phase variations. In the power spectrum, these frequencies also show up…

Astrophysics · Physics 2009-11-11 M. Breger , A. A. Pamyatnykh

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…

The multi-color CCD photometric study of 27 Delta Scuti stars is presented. By using approximately three years of photometric observations, we obtained the times of maxima and magnitude changes during the observation time interval for each…

A study of the star KIC5892969 observed by the Kepler satellite is presented. Its three highest amplitude modes present a strong amplitude modulation. The aim of this work is to investigate amplitude variations in this star and their…

Solar and Stellar Astrophysics · Physics 2015-07-22 S. Barceló Forteza , E. Michel , T. Roca Cortés , R. A. García

The CoRoT mission is in its third year of observation and the data from the second long run in the galactic centre direction are being analysed. The solar-like oscillating stars that have been observed up to now have given some interesting…

This paper examines the 46 frequencies found in the Delta Sct star KIC 8054146 involving a frequency spacing of exactly 2.814 c/d (32.57 microHz), which is also a dominant low-frequency peak near or equal to the rotational frequency. These…

Solar and Stellar Astrophysics · Physics 2015-06-16 M. Breger , P. Lenz , A. A. Pamyatnykh

We present the first catalogue of double-mode and multi-mode high amplitude $\delta$ Scuti star (HADS) in the Galaxy. The catalogue contains source name, coordinates, radial modes such as the fundamental (F, period P0), first-overtone (1O,…

Solar and Stellar Astrophysics · Physics 2021-10-27 Tao-Zhi Yang , Zhao-Yu Zuo , Xin-Yue Wang , Xiao-Ya Sun , Rui-Xuan Tang

Seismology of single delta Scuti stars has mainly been inhibited by failing to detect many of the theoretically predicted pulsation modes, resulting in difficulties with mode identification. Theoretical and observational advances have,…

Astrophysics · Physics 2008-11-04 Orlagh L. Creevey

People can diagnose the interiors of stars by sensing their pulsations. Pulsation modes, which are determined by the internal state and structure of a star, are typically considered stable over short timescales. These independent pulsation…

Solar and Stellar Astrophysics · Physics 2024-02-13 Jia-Shu Niu , Hui-Fang Xue

We have made an asteroseismic analysis of the variable blue stragglers in the open cluster M67. The data set consists of photometric time series from eight sites using nine 0.6-2.1 meter telescopes with a time baseline of 43 days. In two…

We present an analysis of new Johnson and Stromgren photometric and medium-resolution spectroscopic observations of the delta Scuti type variable star V784 Cassiopeae. The data were obtained in three consecutive years between 1999 and 2001.…

Astrophysics · Physics 2009-03-09 L. L. Kiss , A. Derekas , E. J. Alfaro , I. B. Biro , B. Csak , R. Garrido , K. Szatmary , J. R. Thomson

The rapidly increasing number of delta Scuti stars with regular patterns among their pulsation frequencies necessitates modelling tools to better understand the observations. Further, with a dozen identified modes per star, there is…

Solar and Stellar Astrophysics · Physics 2023-09-14 Simon J. Murphy , Timothy R. Bedding , Anuj Gautam , Meridith Joyce

This paper examines the mode identification and presents pulsation models for FG Vir, for which 24 frequencies have been detected. Histograms of the frequency spacings show peaks which are identified with adjacent radial orders and…

Astrophysics · Physics 2007-05-23 M. Breger , A. A. Pamyatnykh , H. Pikall , R. Garrido

The frequency ratios and of HD 49933 exhibit an increase at high frequencies. This behavior also exists in the ratios of other stars, which is considered to result from the low signal-to-noise ratio and the larger line width at the…

Solar and Stellar Astrophysics · Physics 2015-06-18 Zhie Liu , Wuming Yang , Shaolan Bi , Zhijia Tian , Kang Liu , Zhishuai Ge , Jie Yu , Tanda Li , Xiaoyan Tan , Xin He , Yaqian Wu , P. Chintarungruangchai
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