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We present an advance in the use of Cassini observations of stellar occultations by the rings of Saturn for stellar studies. Stewart et al. (2013) demonstrated the potential use of such observations for measuring stellar angular diameters.…

天体物理仪器与方法 · 物理学 2015-03-30 Paul N. Stewart , Peter G. Tuthill , Philip D. Nicholson , Matthew M. Hedman , James P. Lloyd

We obtain the largest catalog of multi-mode $\delta$ Sct stars in the northern sky to date using the Zwicky Transient Facility (ZTF) Data Release 20 (DR20). The catalog includes 2254 objects, of which 2181 are new to our study. Among these…

太阳与恒星天体物理 · 物理学 2024-05-27 Qi Jia , Xiaodian Chen , Shu Wang , Licai Deng , Yangping Luo , Qingquan Jiang

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…

天体物理学 · 物理学 2009-11-13 P. Lenz , A. A. Pamyatnykh , M. Breger , V. Antoci

We present photometric and spectroscopic follow-up observations of short-period variables discovered in the OmegaWhite survey: a wide-field high-cadence g-band synoptic survey targeting the Galactic Plane. We have used fast photometry on…

We present high precision CCD photometry of 1791 objects in 20 open clusters with an age from 10 Myr to 1 Gyr. These observations were performed within the Delta a photometric system which is primarily used to detect chemically peculiar…

天体物理学 · 物理学 2009-11-10 E. Paunzen , K. Zwintz , H. M. Maitzen , O. I. Pintado , M. Rode-Paunzen

Dome A on the Antarctic plateau is likely one of the best observing sites on Earth thanks to the excellent atmospheric conditions present at the site during the long polar winter night. We present high-cadence time-series aperture…

We report a simultaneous ground and space-based photometric study of the Beta Cephei star Nu Eridani. Half a year of observations have been obtained by four of the five satellites constituting BRITE-Constellation, supplemented with…

Frequencies of 13 oscillation modes in the star XX Pyxidis (CD-24 7599) are accurately measured but for none of the modes the spherical harmonic degree l is known. We present results of an attempt to construct the model whose low-l mode…

天体物理学 · 物理学 2007-05-23 A. A. Pamyatnykh , W. A. Dziembowski , G. Handler , H. Pikall

The beta Cephei star delta Ceti was considered one of the few monoperiodic variables in the class. Despite (or perhaps because of) its apparently simple oscillation spectrum, it has been challenging and controversial to identify this star's…

We analyze data on pulsation amplitudes and phases for two $\beta$ Cephei stars, $\delta$ Cet and $\nu$ Eri. Str\"omgren photometry and radial velocity measurements are used simultaneously to obtain constraints on mean parameters of the…

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

We have analysed the photometric data obtained with the STEREO spacecraft for 558 non-magnetic chemically peculiar (CP) stars to search for rotational and pulsational variability. Applying the Lomb-Scargle and the phase dispersion…

太阳与恒星天体物理 · 物理学 2015-06-12 E. Paunzen , K. T. Wraight , L. Fossati , M. Netopil , G. J. White , D. Bewsher

Delta Scuti ($\delta$ Sct) stars are intermediate-mass pulsators, whose intrinsic oscillations have been studied for decades. However, modelling their pulsations remains a real theoretical challenge, thereby even hampering the precise…

We describe a high speed time-series CCD photometer for the prime focus of the 82-in (2.1 m) telescope at McDonald Observatory, and summarize the observational results we have obtained since it was placed into regular use in February, 2002.…

天体物理学 · 物理学 2009-11-07 R. E. Nather , Anjum. S. Mukadam

Pulsating variable $\delta$ Scuti stars are intermediate-mass stars with masses in the range of $1-3$ $M_{\odot}$ and spectral types between $A2$ and $F2$. They can be found at the intersection of the Cepheid instability strip with the main…

太阳与恒星天体物理 · 物理学 2023-09-11 Mami Deka , Shashi M. Kanbur , Sukanta Deb , Susmita Das

The frequency of pressure (p) mode in $\delta$~Scuti stars can exceed the Nyquist limit of \textit{Kepler} long-cadence photometry. {These 'super-Nyquist frequencies' (SNFs) are observed as 'reflected' peaks at lower frequencies, i.e., they…

太阳与恒星天体物理 · 物理学 2026-05-06 Yanqi Mo , Weikai Zong , Xuan Wang , Simon Murphy , Zilu Yang , Jian-Ning Fu , Stephane Charpinet , Xiao-Yu Ma

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

$\delta$ 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 construct seismic models of the four double-mode radial $\delta$ Scuti stars adopting opacities from three databases: OPAL, OP and OPLIB. The aim is to find the models that fit the observed frequencies of the two radial modes and have…

The aspects of the analysis of photometric time-series obtained on double-mode or multiperiodic pulsating stars are briefly reviewed. In particular, the ratios between frequencies are used to pin cases revealing peculiarities. In addition…

天体物理学 · 物理学 2009-11-10 Ennio Poretti , Marco Beltrame