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We present $V,I$ light curves for 12 variable stars identified in the newly discovered satellite of the Milky Way in the Bootes constellation (Belokurov et al. 2006).Our sample includes 11 RR Lyrae stars (5 first overtone, 5 fundamental…

The ninth part of the OGLE-III Catalog of Variable Stars (OIII-CVS) comprises RR Lyr stars in the Small Magellanic Cloud (SMC). Our sample consists of 2475 variable stars, of which 1933 pulsate in the fundamental mode (RRab), 175 are the…

太阳与恒星天体物理 · 物理学 2010-09-29 I. Soszynski , A. Udalski , M. K. Szymanski , M. Kubiak , G. Pietrzynski , L. Wyrzykowski , K. Ulaczyk , R. Poleski

RR Lyrae stars are one of the primary distance indicators for old stellar populations such as globular clusters, dwarf galaxies and galaxies. Typically, fundamental-mode RR Lyr stars are used for distance measurements, and their accuracy is…

太阳与恒星天体物理 · 物理学 2023-06-21 Xiaodian Chen , Jianxing Zhang , Shu Wang , Licai Deng

Radial velocities of fifteen double-mode bulge RR Lyrae (RR01) stars are presented, six of which belong to a compact group of RR01 stars in pulsation space, with the ratio of first-overtone period to fundamental-mode period,…

We present the results of a photometric study of RR Lyrae variables in the field of the globular cluster M55. We have discovered nine new RR Lyrae stars, increasing the number of known variables in this cluster to 15 objects. Five of the…

天体物理学 · 物理学 2009-10-31 A. Olech , J. Kaluzny , I. B. Thompson , W. Pych , W. Krzeminski , A. Schwarzenberg-Czerny

We present the catalog of RR Lyrae stars from 2.4 square degrees of central parts of the Small Magellanic Cloud (SMC). The photometric data were collected during four years of the OGLE-II microlensing survey. Photometry of each star was…

RR Lyrae stars have long been considered reliable tracers of old, metal-poor populations, primarily due to their prevalence in globular clusters and the Galactic halo. However, the discovery of a metal-rich subpopulation in the Galactic…

太阳与恒星天体物理 · 物理学 2025-10-24 HanYuan Zhang , Giuliano Iorio , Vasily Belokurov , N. Wyn Evans , Alexey Bobrick , Valentina D'Orazi

In this paper we report the discovery of 35 new RR Lyrae variables. These stars were found by a special searching technique. We crossmatched the catalog of the PanSTARRS (PS) sky survey with K2 space photometry data to the validate…

太阳与恒星天体物理 · 物理学 2018-03-28 Áron L. Juhász , László Molnár

The second Gaia data release is expected to contain data products from about 22 months of observation. Based on these data, we aim to provide an advance publication of a full-sky Gaia map of RR Lyrae stars. Although comprehensive, these…

We present the detection of RR Lyrae variable stars in the field of the Sagittarius II (Sgr II) ultra-faint dwarf (UFD) galaxy. Using B, V time-series photometry obtained with the Korea Microlensing Telescope Network (KMTNet) 1.6 m…

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

A detailed analysis is presented of 33 RR Lyrae stars in Pisces observed with the Kepler space telescope over the 8.9-day long K2 Two-Wheel Concept Engineering Test. The sample includes not only fundamental-mode and first overtone (RRab and…

太阳与恒星天体物理 · 物理学 2015-08-19 L. Molnár , R. Szabó , P. A. Moskalik , J. M. Nemec , E. Guggenberger , R. Smolec , R. Poleski , E. Plachy , K. Kolenberg , Z. Kolláth

In this article, we present results based on high-density, high-precision Wide-Angle Search for Planets (WASP) light curves supplemented with lower-precision photometry from the All-Sky Automated Survey (ASAS) for 268 RR Lyrae stars (176…

太阳与恒星天体物理 · 物理学 2014-10-22 Marek Skarka

We present the first CCD variability study of the Draco dwarf spheroidal galaxy. The data were obtained with the FLWO 1.2 m telescope on 22 nights, over a period of 10 months, covering a 22 x 22 arcmin field centered at RA=17:19:57.5,…

天体物理学 · 物理学 2008-11-26 A. Z. Bonanos , K. Z. Stanek , A. H. Szentgyorgyi , D. D. Sasselov , G. A. Bakos

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

A century of observations of omega Centauri allows us to accurately follow the period changes of a large sample of variable stars. Although the period changes are composed of monotone and irregular changes, period increases dominate in most…

天体物理学 · 物理学 2009-10-31 Johanna Jurcsik , Christine Clement , Edward H. Geyer , Istvan Domsa

We present a sample of ~5,000 RR Lyrae stars selected from the recalibrated LINEAR dataset and detected at heliocentric distances between 5 kpc and 30 kpc over ~8,000 deg^2 of sky. The coordinates and light curve properties, such as period…

We present a search and analysis of variable stars in the recently discovered Crater~II dwarf galaxy. Based on $B$, $V$, $I$ data collected with the Isaac Newton Telescope (FoV$\sim$0.44 square degrees) we detected 37 variable stars, of…

We present a comprehensive catalog of 2824 RR Lyrae stars (RRLs) residing in 115 Galactic globular clusters (GCs). Our catalog includes 1594 fundamental-mode (RRab), 824 first-overtone (RRc), and 28 double-mode (RRd) RRLs, as well as 378…

太阳与恒星天体物理 · 物理学 2024-02-15 Mauricio Cruz Reyes , Richard I. Anderson , Lucas Johansson , Henryka Netzel , Zoé Medaric

The Kepler space telescope revealed new, unexpected phenomena in RR Lyrae stars: period doubling and the possible presence of additional modes. Identifying these modes is complicated because they blend in the rich features of the…

太阳与恒星天体物理 · 物理学 2015-06-03 L. Molnár , Z. Kolláth , R. Szabó