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相关论文: Binarity and multiperiodicity in high-amplitude de…

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We present our first results for a sample of southern high-amplitude delta Scuti stars (HADS), based on a spectrophotometric survey started in 2003. For CY Aqr and AD CMi, we found very stable light and radial velocity curves; we confirmed…

天体物理学 · 物理学 2010-12-09 A. Derekas , L. L. Kiss , B. Csak , J. Griffin , C. Lindstrom , Sz. Meszaros , P. Szekely , M. C. B. Ashley , T. R. Bedding

Using TESS 20-sec cadence data, we have discovered an unusual combination of pulsating stars in what we infer to be a binary system. The binary consists of a standard $\delta$ Scuti star with pulsations over the range 32-41 d$^{-1}$; this…

We present new photometric data for seven high-amplitude delta Scuti stars. The observations were acquired between 1996 and 2002, mostly in the Johnson photometric system. For one star (GW UMa), our observations are the first since the…

Aim: The focus of this paper is on two famous but still poorly understood RV Tauri stars: RV Tau and DF Cyg. We aim at confirming their suspected binary nature and deriving their orbital elements to investigate the impact of their orbits on…

Radial velocity curves for 15 bright subdwarf B binary systems have been measured using high precision radial velocity measurements from high S/N optical high-resolution spectra. In addition, two bright sdB stars are discovered to be radial…

天体物理学 · 物理学 2009-11-11 H. Edelmann , U. Heber , M. Altmann , C. Karl , T. Lisker

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…

Searching for main-sequence pulsators, we analyzed photometry of ~200,000 variable star candidates from the OGLE-II Galactic fields, finding 193 high-amplitude Delta Scuti stars. This doubles the number of known stars of this type. The…

天体物理学 · 物理学 2010-12-09 A. Pigulski , Z. Kolaczkowski , T. Ramza , A. Narwid

We have used the HIRES echelle spectrograph in the Keck I telescope to obtain high-resolution spectroscopy of 51 late-type M dwarfs in the Hyades cluster. Cross-correlating the calibrated data against spectra of white dwarfs allows us to…

天体物理学 · 物理学 2015-06-24 I. N. Reid , S. Mahoney

A field star, HD 61199 (V ~ 8), simultaneously observed with Procyon by the MOST (Microvariability & Oscillations of STars) satellite in continuous runs of 34, 17, and 34 days in 2004, 2005, and 2007, was found to pulsate in 11 frequencies…

We report the analysis of high temporal resolution ground and space based photometric observations of SZ Lyncis, a binary star one of whose components is a high amplitude $\delta$ Scuti. UBVR photometric observations were obtained from Mt.…

太阳与恒星天体物理 · 物理学 2020-12-23 J. Adassuriya , S. Ganesh , J. L. Gutierrez , G. Handler , Santosh Joshi , K. P. S. C. Jayaratne , K. S. Baliyan

We analyzed period changes of the high-amplitude Delta Scuti variable star CSS_J102714.3+205943 for about 20 years, utilizing data from the automated sky surveys along with our own observations. With the help of the O-C diagram, we found…

太阳与恒星天体物理 · 物理学 2025-05-27 Maksym Yu. Pyatnytskyy , Ivan L. Andronov

In this work, we present a study on the long time-scale period variations of four single-mode high-amplitude delta Scuti stars (HADS) via the classical $O-C$ analysis. The target HADS are (i) XX Cygni, (ii) YZ Bootis, (iii) GP Andromedae,…

太阳与恒星天体物理 · 物理学 2025-04-22 Tian-Fang Ma , Jia-Shu Niu , Hui-Fang Xue

The two stars that form the subject of this paper are both short-period double- lined eclipsing binaries having non-circular orbits despite their short periods. Although the HD type of HD 152028 is G0, the integrated spectral type of the…

天体物理学 · 物理学 2007-05-23 R. F. Griffin , H. M. J. Boffin

We present the spectroscopic orbits of eleven nearby, mid-to-late M dwarf binary systems in a variety of configurations: two single-lined binaries (SB1s), seven double-lined binaries (SB2s), one double-lined triple (ST2), and one…

We present the results of a multi-site photometric campaign carried out in 2004-2008 for the Algol-type eclipsing binary system CT Her, the primary component of which shows Delta Scuti-type oscillations. Our data consist of differential…

Although delta Scorpii is a bright and well-studied star, the details of its multiplicity have remained unclear. Here we present the first diffraction-limited image of this 0.12 arcsec binary star, made using optical interferometry, and…

天体物理学 · 物理学 2009-10-22 Timothy R. Bedding

A subclass of intermediate mass variables Delta Scuti stars, known as High-amplitude Delta Scuti (HADS) stars, exhibits pronounced radial pulsations with high amplitudes. The ground-based and space-based observations of the HADS star EH Lib…

太阳与恒星天体物理 · 物理学 2025-07-22 Xiran Xie , Jianning Fu , Gang Meng , Lester Fox Machado , Raúl Michel , Huifang Xue , Nian Liu , Zhongyang Liu , Jie Su , Mingfeng Qin

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

We used high-quality Kepler photometry and spectroscopic data to investigate the Kepler binary candidate KIC 5988140. Using the spectrum synthesis method, we derived the fundamental parameters Teff, log g, [M/H], and v.sini and the…

We present the most precise to date orbital and physical parameters of the well known short period (P=5.975 d), eccentric (e=0.3) double-lined spectroscopic binary BY Draconis, a prototype of a class of late-type, active, spotted flare…

太阳与恒星天体物理 · 物理学 2015-05-30 K. G. Hełminiak , M. Konacki , M. W. Muterspaugh , S. E. Browne , A. W. Howard , S. R. Kulkarni
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