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We present the results of a photometric survey for variable stars in the central region of the nearby globular cluster NGC 6397.Time series photometry was obtained for 30 variable objects. The sample includes 12 new objects, of which 6 show…

Astrophysics · Physics 2009-11-13 J. Kaluzny , I. B. Thompson , W. Krzeminski

We present time-series B, V photometry of NGC 6229, obtained with the purpose of providing the first extensive CCD variability study of this cluster. As a result, we were able to obtain periods for all NGC 6229 variables, with the exception…

Astrophysics · Physics 2015-06-24 J. Borissova , M. Catelan , T. Valchev

This work presents the first large-scale photometric variability survey of the intermediate age (~200 Myr) open cluster M11. Thirteen nights of data over two observing seasons were analyzed (using crowded field and ensemble photometry…

Astrophysics · Physics 2008-11-26 Jonathan R. Hargis , Eric L. Sandquist , David H. Bradstreet

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…

Solar and Stellar Astrophysics · Physics 2018-03-28 Áron L. Juhász , László Molnár

We present the results of a search for variable stars in the globular cluster NGC 5286, which has recently been suggested to be associated with the Canis Major dwarf spheroidal galaxy. 57 variable stars were detected, only 19 of which had…

A spectroscopic support survey of 103 objects observed by the MOST satellite is presented; 96 are variable stars with 83 of them being new MOST variable-star detections or stars with variability types verified and/or modified on the basis…

This paper presents the first optical variability study of the Westerlund 1 super star cluster in search of massive eclipsing binary systems. A total of 129 new variable stars have been identified, including the discovery of 4 eclipsing…

Astrophysics · Physics 2008-11-26 Alceste Z. Bonanos

We have applied the image subtraction method to images of the peculiar, bimodal-horizontal branch globular cluster NGC 2808, taken over a total of six nights over a range of five months. As a result, we have found, for the first time, a…

Astrophysics · Physics 2009-11-10 T. M. Corwin , M. Catelan , J. Borissova , H. A. Smith

We identify 228 periodic variables in the region of young open cluster NGC 281 using time series photometry carried out from 1 m class ARIES telescopes, Nainital. The cluster membership of these identified variables is determined on the…

Solar and Stellar Astrophysics · Physics 2021-04-21 Sneh Lata , A. K. Pandey , J. C. Pandey , Neelam Panwar , Paulomi Paul

We present the second part of the OGLE Catalog of Periodic Variable Stars in the Galactic bulge. 800 variable stars found in four Baade's Window fields BW1, BW2, BW3 and BW4 are presented. Among them 71 are classified as pulsating, 465 as…

Astrophysics · Physics 2007-05-23 A. UDALSKI , M. SZYMANSKI , J. KALUZNY , M. KUBIAK , M. MATEO , W. KRZEMINSKI

The Quintuplet cluster is one of the most massive star clusters in the Milky Way, situated very close to the Galactic center. We present a new search for variable stars in the vicinity of the cluster, using the five-year database of the…

Solar and Stellar Astrophysics · Physics 2016-07-26 C. Navarro Molina , J. Borissova , M. Catelan , J. Alonso-García , E. Kerins , R. Kurtev , P. W. Lucas , N. Medina , D. Minniti , I. Dékány

We present new B, V and I CCD time-series photometry for 177 variable stars in a 13'X 13' field centered on the globular cluster M54 (lying at the center of the Sagittarius dwarf spheroidal galaxy), 94 of which are newly identified…

Astrophysics of Galaxies · Physics 2015-05-18 A. Sollima , C. Cacciari , M. Bellazzini , S. Colucci

We report an analysis of new $V$ and $I$ CCD time-series photometry of the globular cluster NGC 6934. Through the Fourier decomposition of the RR Lyrae light curves, the mean values of [Fe/H] and the distance of the cluster were estimated,…

Solar and Stellar Astrophysics · Physics 2017-09-04 M. A. Yepez , A. Arellano Ferro , S. Muneer , Sunetra Giridhar

We present time-series VI photometry of the metal-rich ([Fe/H] = -0.53) globular cluster NGC 6441. Our color-magnitude diagram shows that the extended blue horizontal branch seen in Hubble Space Telescope data exists in the outermost…

Astrophysics · Physics 2009-10-30 A. C. Layden , L. A. Ritter , D. L. Welch , T. M. A. Webb

We have identified some two-hundred new variable stars in a systematic study of a data archive obtained with the Calvin-Rehoboth observatory. Of these, we present five close binaries showing behaviors presumably due to star spots or other…

Solar and Stellar Astrophysics · Physics 2013-10-03 Steven D. Steenwyk , Daniel M. Van Noord , Lawrence A. Molnar

Based on over 3000 BV images of M4 collected in years 1995-2009 we obtain light curves of 22 variables, 10 of which are newly detected objects. We identify four detached eclipsing binaries and eight contact binaries. Accurate periods are…

Solar and Stellar Astrophysics · Physics 2013-07-15 J. Kaluzny , I. B. Thompson , M. Rozyczka , W. Krzeminski

We have conducted a deep photometric survey of a 0.5 deg x 0.5 deg area of the Galactic Plane using the WFI instrument on the 2.2-m ESO telescope on La Silla, Chile. The dataset comprises a total of 267 R-band images, 204 from a 16 day…

Solar and Stellar Astrophysics · Physics 2015-05-19 V. R. Miller , M. D. Albrow , C. Afonso , Th. Henning

We present the analysis of 11 589 eclipsing binary stars identified in twenty-one OGLE-III Galactic disk fields toward constellations of Carina, Centaurus, and Musca. All eclipsing binaries but 402 objects are new discoveries. The binaries…

We describe an ongoing variable star search program and present the first reduced results of a search in a 19 square degree (4.4\circle x 4.4\circle) field centered on J2000 {\alpha} = 22:03:24, {\delta} = +18:54:32. The search was carried…

Astrophysics of Galaxies · Physics 2011-02-01 Michael D. Williams , E. F. Milone

The COROT space mission will monitor several target fields for up to 150 days to perform asteroseismology and to search for extrasolar planets by photometric transits. Variable stars in the target fields are important objects for additional…

Solar and Stellar Astrophysics · Physics 2009-09-29 C. Karoff , H. Rauer , A. Erikson , H. Voss , P. Kabath , T. Wiese , M. Deleuil , C. Moutou , J. C. Meunier , H. Deeg