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Related papers: On the Oosterhoff dichotomy in the Galactic bulge:…

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We present a sample of 209 variable objects - very likely optical counterparts to the X-ray sources detected in the direction of the Galactic center by the Galactic Bulge Survey (GBS) carried out with the Chandra satellite. The variable…

We report the discovery of a new group of double-periodic RR Lyrae stars from the analysis of the OGLE-IV Galactic bulge photometry. In 11 stars identified in the OGLE catalog as first overtone pulsators (RRc stars) we detect additional…

Solar and Stellar Astrophysics · Physics 2015-05-14 H. Netzel , R. Smolec , W. Dziembowski

CONTEXT. This is the second paper of a series on Galactic OB groups that uses astrometric and photometric data from Gaia and spectral classifications from GOSSS and LiLiMaRlin. The previous paper was based on Gaia DR2, this is based on Gaia…

Deep near-IR images from the VISTA Variables in the V\'ia L\'actea (VVV) Survey were used to search for RR Lyrae stars in the Southern Galactic plane. A sizable sample of 404 RR Lyrae of type ab stars was identified across a thin slice of…

We analyse the OGLE-IV photometry of the first overtone and double-mode RR Lyrae stars (RRc/RRd) in the two fields towards the Galactic bulge observed with high cadence. In 27 per cent of RRc stars we find additional non-radial mode, with…

Solar and Stellar Astrophysics · Physics 2015-09-01 H. Netzel , R. Smolec , P. Moskalik

We present a collection of 65,981 Mira-type variable stars found in the Optical Gravitational Lensing Experiment (OGLE) project database. Two-thirds of our sample (40,356 objects) are located in the Galactic bulge fields, whereas 25,625…

We present a collection of classical, type II, and anomalous Cepheids detected in the OGLE fields toward the Galactic center. The sample contains 87 classical Cepheids pulsating in one, two or three radial modes, 924 type II Cepheids…

We present a catalog of 1888 fundamental-mode RR Lyrae stars detected in the Galactic bulge fields of the second phase of the Optical Gravitational Lensing Experiment (OGLE). The catalog includes basic parameters of the light curves,…

Astrophysics · Physics 2008-11-26 Matthew J. Collinge , Takahiro Sumi , Daniel Fabrycky

We present results of star variability analysis in OGLE II first bulge field. Photometric database was derived by means of image subtraction method (Wozniak 2000) and contains 4597 objects pre-classified as variables. We analyzed all the…

Astrophysics · Physics 2007-05-23 Tomasz Mizerski , Michal Bejger

We present a statistical assessment of both, observed and reported, photometric uncertainties in the OGLE-IV Galactic bulge microlensing survey data. This dataset is widely used for the detection of variable stars, transient objects,…

Instrumentation and Methods for Astrophysics · Physics 2016-04-08 J. Skowron , A. Udalski , S. Kozłowski , M. K. Szymański , P. Mróz , Ł. Wyrzykowski , R. Poleski , P. Pietrukowicz , K. Ulaczyk , M. Pawlak , I. Soszyński

We present an analysis of the structure, kinematics, and chemo-dynamical properties of the Milky Way bulge using RR Lyrae stars from OGLE, and giant stars from APOGEE and Gaia that have distances placing them in the inner Galaxy. Firstly,…

Astrophysics of Galaxies · Physics 2025-03-25 Xiao Han , Hai-Feng Wang , Giovanni Carraro , Martín López-Corredoira , Yuan-Sen Ting , Yang-Ping Luo , Guan-Yu Wang

The fifteenth part of the OGLE-III Catalog of Variable Stars (OIII-CVS) contains 232,406 long-period variables (LPVs) detected in the OGLE-II and OGLE-III fields toward the Galactic bulge. The sample consists of 6528 Mira stars, 33,235…

We re-examine the Bailey diagrams of fundamental mode RR Lyrae stars from the perspective of horizontal branch (HB) evolution, identifying evolutionary effects as the probable direct cause of the Oosterhoff dichotomy. By establishing…

Solar and Stellar Astrophysics · Physics 2025-09-11 L. -J. Li , S. -B. Qian , L. -Y. Zhu , X. -D. Shi , W. -P. Liao

We report the discovery of a significant population of RR Lyrae variables in the dwarf spheroidal galaxy Leo I. Based on 40 V and 22 B images of the galaxy taken using the ESO Wide Field Imager we have identified so far 74 candidate RR…

Astrophysics · Physics 2009-11-07 E. V. Held , G. Clementini , L. Rizzi , Y. Momany , I. Saviane , L. Di Fabrizio

We present the Catalog of microlensing events detected toward the Galactic bulge in three observing seasons, 1997--1999, during the OGLE-II microlensing survey. The search for microlensing events was performed using a database of about…

Astrophysics · Physics 2007-05-23 A. Udalski , K. Zebrun , M. Szymanski , M. Kubiak , G. Pietrzynski , I. Soszynski , P. Wozniak

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…

Astrophysics · Physics 2009-11-07 P. Moskalik , E. Poretti

We analyse photometry of $\sim$2000 Galactic Cepheids available in the OGLE Collection of Variable Stars. We analyse both Galactic disk and Galactic bulge fields; stars classified both as single- and multi-periodic. Our goal was to search…

Solar and Stellar Astrophysics · Physics 2021-07-07 R. S. Rathour , R. Smolec , H. Netzel

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…

Solar and Stellar Astrophysics · Physics 2024-02-15 Mauricio Cruz Reyes , Richard I. Anderson , Lucas Johansson , Henryka Netzel , Zoé Medaric

We present 20 newly discovered candidates for binary systems with an RR~Lyrae companion. Using the photometric data from the Optical Gravitational Lensing Experiment (OGLE) and Korea Microlensing Telescope Network (KMTNet) for the Galactic…

Solar and Stellar Astrophysics · Physics 2019-06-05 Z. Prudil , M. Skarka , J. Liška , E. K. Grebel , C. -U. Lee

We present a theoretical investigation on the pulsational behavior of metal-rich RR Lyrae variables over the range of evolutionary parameters suitable for stars with metallicities Z= 0.006, 0.01 and 0.02. With the addition of similar…

Astrophysics · Physics 2009-10-30 Giuseppe Bono , Filippina Caputo , Santi Cassisi , Roberta Incerpi , Marcella Marconi