中文
相关论文

相关论文: Double-Mode RR Lyrae Stars Observed by K2: Analysi…

200 篇论文

We present the results of the analysis of Type II and anomalous Cepheids using the data from the Kepler K2 mission. The precise light curves of these pulsating variable stars are the key to study the details of their pulsation, such as the…

We have examined the period-luminosity (P-L) relation for delta Scuti stars using Gaia DR2 parallaxes. We included 228 stars from the catalogue of Rodriguez et al. (2000), as well as 1124 stars observed in the four-year Kepler mission. For…

太阳与恒星天体物理 · 物理学 2019-04-30 Elham Ziaali , Timothy R. Bedding , Simon J. Murphy , Timothy Van Reeth , Daniel R. Hey

Context. The multiplicity of classical Cepheids (CCs) and RR Lyrae stars (RRLs) is still imperfectly known, particularly for RRLs. Aims. In order to complement the close-in short orbital period systems presented in Paper I, our aim is to…

太阳与恒星天体物理 · 物理学 2019-08-05 P. Kervella , A. Gallenne , N. R. Evans , L. Szabados , F. Arenou , A. Mérand , N. Nardetto , W. Gieren , G. Pietrzynski

Period study of 321 fundamental mode galactic field RR Lyrae type stars (RRab), which had appropriate data in ASAS and SuperWASP surveys, brighter than 12.5 mag in maximum light was performed. We found 100 stars to be definitely modulated.…

太阳与恒星天体物理 · 物理学 2015-06-18 Marek Skarka

We report the discovery of 73 double-mode RR Lyrae (RRd) stars in fields near the bar of the LMC. The stars are detected among the MACHO database of short-period variables that currently contains about 7900 RR Lyrae stars. Fundamental…

We combine observed metallicity, optical and infrared magnitudes with evolutionary and pulsation models to derive average luminosities for 156 single-mode RR Lyrae stars. These luminosities are compared with those obtained from the Gaia…

太阳与恒星天体物理 · 物理学 2021-10-13 Geza Kovacs , Behrooz Karamiqucham

We present a comprehensive photometric study of RR Lyrae stars in the M3 globular cluster, utilising a vast dataset of 3140 optical ($UBVRI$) CCD images spanning 35 years from astronomical data archives. We have successfully identified…

太阳与恒星天体物理 · 物理学 2024-05-28 Nitesh Kumar , Anupam Bhardwaj , Harinder P. Singh , Marina Rejkuba , Marcella Marconi , Philippe Prugniel

We determine the fundamental stellar parameters of altogether 20 double-mode RR Lyrae (RRd) stars from the Galactic Field and the Large Magellanic Cloud, following our approach employed on the field RRd star BS Comae. The stars were…

太阳与恒星天体物理 · 物理学 2015-05-13 Istvan Dekany

We have started a comprehensive analysis of the Kepler K2 Field 3 data set. Our goals are to assess the statistics of the sample, and to search for peculiar stars. We found a candidate triple-mode RRab star, where the first and ninth…

太阳与恒星天体物理 · 物理学 2016-03-30 Á. Juhász , L. Molnár , E. Plachy

The origin of the conspicuous amplitude and phase modulation of the RR Lyrae pulsation - known as the Blazhko effect - is still a mystery after more than 100 years of its discovery. With the help of the Kepler space telescope we have…

太阳与恒星天体物理 · 物理学 2015-06-03 R. Szabó , Z. Kolláth , L. Molnár , K. Kolenberg , D. W. Kurtz , WG#13 members

The first detection of the period doubling phenomenon is reported in the Kepler RR Lyrae stars RR Lyr, V808 Cyg and V355 Lyr. Interestingly, all these pulsating stars show Blazhko modulation. The period doubling manifests itself as…

We have frequency analyzed 6391 variables classified earlier as fundamental mode RR Lyrae (RR0) stars in the MACHO database on the Large Magellanic Cloud (LMC). The overwhelming majority of these variables have been proved to be indeed RR0…

V473 Lyrae is the only Galactic Cepheid with confirmed periodic amplitude and phase variations similar to the Blazhko effect observed in RR Lyrae stars. We collected all available photometric data and some radial velocity measurements to…

太阳与恒星天体物理 · 物理学 2015-06-19 László Molnár , László Szabados

The Gaia second Data Release (DR2) presents a first mapping of full-sky RR Lyrae stars and Cepheids observed by the spacecraft during the initial 22 months of science operations. The Specific Object Study (SOS) pipeline, developed to…

Gaia DR3 publishes a catalogue of full-sky RR Lyrae stars (RRLs) observed during the initial 34 months of science operations, that were processed through the Specific Object Study (SOS) pipeline for Cepheids and RRLs (SOS Cep&RRL) observed…

We document the presence of a few Cepheid and RR Lyrae variable stars with previously unrecognized characteristics. These stars exhibit the property of a period ratio of main pulsation divided by secondary pulsation P1/P2 very close to…

太阳与恒星天体物理 · 物理学 2014-09-17 Michael Hippke , John G. Learned , A. Zee

We present an analysis of \emph{VI} CCD time-series photometry of the Oo II type globular cluster M92. The variable star population of the cluster is studied with the aim of revising their classifications, identifications, frequency spectra…

太阳与恒星天体物理 · 物理学 2020-03-18 M. A. Yepez , A. Arellano Ferro , D. Deras

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 present the results of a systematic search for multiperiodic pulsators among the Galactic Bulge RR Lyrae stars of the OGLE-1 sample. We identify one "canonical" double-mode variable (RRd star) pulsating in two radial modes. In 38 stars…

天体物理学 · 物理学 2009-11-07 P. Moskalik , E. Poretti

42 RRab, 46 RRc and 7 previously unidentified double-mode RR Lyrae stars were found in the publicly available data of the WASP archive. The Galactic double-mode RR Lyrae stars appear to show a bimodal period distribution.

太阳与恒星天体物理 · 物理学 2010-11-08 Patrick Wils