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相关论文: Toward mode selection in Delta Scuti stars: Regula…

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The high accuracy of space data increased the number of the periodicities determined for pulsating variable stars, but the mode identification is still a critical point in the non-asymptotic regime. We use regularities in frequency spacings…

太阳与恒星天体物理 · 物理学 2015-06-16 M. Paparo , Zs. Bognar , J. M. Benko , D. Gandolfi , A. Moya , J. C. Suarez , A. Sodor , M. Hareter , E. Poretti , E. W. Guenther , M. Auvergne , A. Baglin , W. W. Weiss

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…

Asteroseismology is a powerful tool for probing the internal structures of stars by using their natural pulsation frequencies. It relies on identifying sequences of pulsation modes that can be compared with theoretical models, which has…

The majority of the well-studied Delta Scuti stars show frequency pairs in the power spectra with frequency separations less than 0.06 c/d(0.7 microHz) as well as amplitude variability. We examine the interpretation in terms of separate…

天体物理学 · 物理学 2009-11-07 M. Breger , K. M. Bischof

We discuss the results of a systematic search for multiperiodic pulsations in Galactic Bulge Delta Scuti and RR Lyrae stars. Six "normal" double-mode variables pulsating in two radial modes have been identified (5 Delta Scuti-type and 1 RR…

天体物理学 · 物理学 2007-05-23 P. Moskalik , E. Poretti

The nature of period and amplitude changes in nonradial pulsators is presently unknown. It is therefore important to examine the correlations between these changes in stars with a large number of simultaneously excited pulsation modes.…

太阳与恒星天体物理 · 物理学 2016-08-17 Michel Breger

A sequence search method was developed for searching for regular frequency spacing in delta Scuti stars by visual inspection and algorithmic search. The sample contains 90 delta Scuti stars observed by CoRoT. An example is given to…

太阳与恒星天体物理 · 物理学 2016-06-22 M. Paparó , J. M. Benkő , M. Hareter , J. A. Guzik

Hybrid stars of the {\gamma} Doradus and {\delta} Scuti pulsation types have great potential for asteroseismic analysis to explore their interior structure. To achieve this, mode identi- fications of pulsational frequencies observed in the…

太阳与恒星天体物理 · 物理学 2015-06-23 E. Brunsden , K. R. Pollard , P. L. Cottrell , K. Uytterhoeven , D. J. Wright , P. De Cat

In most Delta Scuti stars, the measured period changes are considerably larger than those expected from stellar evolution. In order to study these period and amplitude changes, a few selected stars are measured photometrically for hundreds…

太阳与恒星天体物理 · 物理学 2015-05-14 Michel Breger

Space-based photometry reveals regular high-frequency patterns in many young $\delta$ Scuti stars. These pulsations provide a powerful means of inferring stellar properties, particularly ages, for young $\delta$ Scuti stars for which…

太阳与恒星天体物理 · 物理学 2026-03-26 Anuj Gautam , Simon J. Murphy , Timothy R. Bedding

Oscillation modes in fast-rotating stars can be split into several subclasses, each with their own properties. To date, seismology of these stars cannot rely on regular pattern analysis and scaling relations. However, recently there has…

太阳与恒星天体物理 · 物理学 2018-11-28 Giovanni M. Mirouh , George C. Angelou , Daniel R. Reese , Guglielmo Costa

Amplitude and phase variability are commonly found in many different types of pulsating stars. This suggests a common, presently unknown physical origin. We have examined the phenomenon in several Delta Scuti stars with extensive data and…

天体物理学 · 物理学 2010-12-09 M. Breger , A. A. Pamyatnykh

We present high-precision time-series photometry of the classical delta Scuti star HD 144277 obtained with the MOST (Microvariability and Oscillations of STars) satellite in two consecutive years. The observed regular frequency patterns are…

$\delta$ Scuti stars are pulsating variable stars that exhibit both radial and non-radial pulsations, making them key objects for understanding stellar evolution and internal structures. The current classification of $\delta$ Scuti stars…

太阳与恒星天体物理 · 物理学 2026-02-03 J. R. Rodon , J. Pascual-Granado , M. Lares-Martiz , M. Rodríguez Sánchez , C. Roche

We present new spectroscopic and photometric time series observations of the delta Scuti star FG~Vir. We detect the oscillations via changes in the equivalent widths of hydrogen and metal absorption lines. From the ratios between…

天体物理学 · 物理学 2007-05-23 M. Viskum , H. Kjeldsen , T. R. Bedding , T. H. Dall , I. K. Baldry , H. Bruntt , S. Frandsen

We use TESS 10-minute Full Frame Images (Sectors 27-55) to study a sample of 1708 stars within 500 pc of the Sun that lie in a narrow colour range in the centre of the delta Scuti instability strip (0.29 < BP-RP < 0.31). Based on the…

{\delta} Scuti variables are found at the intersection of the classical instability strip and the main sequence on the Hertzsprung-Russell diagram. With space-based photometry providing millions of light-curves of A-F type stars, we can now…

太阳与恒星天体物理 · 物理学 2024-05-31 Keyan Gootkin , Marc Hon , Daniel Huber , Daniel R. Hey , Timothy R. Bedding , Simon J. Murphy

In addition to revealing spherical harmonic degrees, $\ell$, of excited modes, pulsational amplitudes and phases from multicolour photometry and radial velocity data yield a valuable constraints on stellar atmospheric parameters and on…

天体物理学 · 物理学 2009-11-10 J. Daszynska-Daszkiewicz , W. A. Dziembowski , A. A. Pamyatnykh , M. Breger , W. Zima

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'

MOST observations and model analysis of the Herbig Ae star HD 34282 (V1366 Ori) reveal {\delta}-Scuti pulsations. 22 frequencies are observed, 10 of which confirm those previously identified by Amado et al. (2006), and 12 of which are newly…