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相关论文: Variable Stars in the Quintuplet stellar cluster w…

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The evolution of massive stars is only partly understood. Observational constraints can be obtained from the study of massive stars located in young massive clusters. The ESO Public Survey VISTA Variables in the Via Lactea (VVV) discovered…

太阳与恒星天体物理 · 物理学 2015-12-23 A. Hervé , F. Martins , A. -N. Chené , J. -C. Bouret , J. Borissova

We have undertaken a long-term project, Planets in Stellar Clusters Extensive Search (PISCES), to search for transiting planets in open clusters. NGC 2158 is one of the targets we have chosen -- an intermediate age, populous, rather metal…

天体物理学 · 物理学 2009-11-10 B. J. Mochejska , K. Z. Stanek , D. D. Sasselov , A. H. Szentgyorgyi , M. Westover , J. N. Winn

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…

This paper presents the Charge-Coupled Device time-series photometric observations of the open cluster NGC 1582 and its surrounding field with Johnson B, V and R filters by using Nanshan 1m telescope of Xinjiang Astronomical Observatory. 19…

太阳与恒星天体物理 · 物理学 2018-09-27 Fang-Fang Song , Ali Esamdin , Lu Ma , Jin-Zhong Liu , Yu Zhang , Hu-Biao Niu , Tao-Zhi Yang

We present results of time series photometry to search for variable stars in the field of metal-poor globular cluster NGC 4590 (M68). Periods have been revised for 40 known variables and no significant changes were found. A considerable…

星系天体物理 · 物理学 2013-09-11 Devesh Path Sariya , Sneh Lata , R. K. S. Yadav

Obtain time-series photometry of the very crowded central regions of Galactic globular clusters with better angular resolution than previously achieved with conventional CCDs on ground-based telescopes to complete, or improve, the census of…

We present the first catalogue of known variable stars in open cluster regions and with up to two times the given cluster radius. This gives basic information about the distribution of variable stars in cluster fields for the complete sky.…

太阳与恒星天体物理 · 物理学 2015-06-12 Miloslav Zejda , Ernst Paunzen , Bernhard Baumann , Zdenek Mikulasek , Jiri Liska

We present the results of a photometric survey for variable stars in the nearby globular cluster M5. A 14.8x22.8 arcmin^2 field centered on the cluster was monitored for a total of 37 hours with a CCD camera mounted on the 1.0-m Swope…

天体物理学 · 物理学 2007-05-23 J. Kaluzny , I. Thompson , W. Krzeminski , W. Pych

We present the results of a variable stars search in the field of the old open cluster NGC 2204. Five new variables were found, four of them being eclipsing binaries. The sample includes a detached binary located at the turnoff, a W UMa -…

天体物理学 · 物理学 2009-06-25 M. Rozyczka , J. Kaluzny , W. Krzeminski , B. Mazur

Using light curves with $\sim$3 min cadence and a duration of 2 hrs made using the OmegaWhite survey, we present the results of a search for short-period variable stars in the field of 20 open clusters. We identified 92 variable stars in…

太阳与恒星天体物理 · 物理学 2022-04-06 R. Toma , G. Ramsay , C. S. Jeffery , S. A. Macfarlane , P. Woudt , P. J. Groot

Despite indications that classical cataclysmic variable (CV) stars are rare in globular clusters in general, and in the cluster NGC 6624 in particular, we have serendipitously discovered such a star ~6'' from the cluster center. A Hubble…

天体物理学 · 物理学 2009-10-31 Eric W. Deutsch , Bruce Margon , Scott F. Anderson , Ronald A. Downes

We present a catalogue of variable stars in the near-infrared wavelength detected with overlapping regions of the 2MASS public images, and discuss their properties. The investigated region is in the direction of the Galactic center (-30 < l…

太阳与恒星天体物理 · 物理学 2014-11-20 Shinjirou Kouzuma , Hitoshi Yamaoka

Time-series data taken with the Hubble Space Telescope of three fields covering the central part of the globular cluster M22 have been analyzed in search of variable objects. We report identification of 11 periodic variables of which 8 are…

天体物理学 · 物理学 2007-05-23 Pawel Pietrukowicz , Janusz Kaluzny

We report the detection of 1143 variable stars towards the Galactic bulge, including 320 previously uncatalogued variables, using time-series photometry extracted from data obtained with the VIMOS imager at the Very Large Telescope.…

太阳与恒星天体物理 · 物理学 2018-10-31 N. Kains , A. Calamida , M. Rejkuba , A. Bhardwaj , L. Inno , K. C. Sahu , M. Zoccali , G. Bono , F. Surot , J. Anderson , S. Casertano

The field of the globular cluster M10 (NGC 6254) was monitored between 1998 and 2015 in a search for variable stars. V -light curves were derived for 40 variables or likely variables, most of which are new detections. Proper motions…

太阳与恒星天体物理 · 物理学 2021-03-10 M. Rozyczka , W. Narloch , A. Schwarzenberg - Czerny , I. B. Thompson , R. Poleski , W. Pych

We present initial results of the first panoramic search for high-amplitude near-infrared variability in the Galactic Plane. We analyse the widely separated two-epoch K-band photometry in the 5th and 7th data releases of the UKIDSS Galactic…

We present a new search for variable stars in the Galactic globular cluster M28 (NGC 6626). The search is based on a series of BVI images obtained with the SMARTS Consortium's 1.3m telescope at Cerro Tololo Inter-American Observatory,…

太阳与恒星天体物理 · 物理学 2015-06-05 G. Prieto , M. Catelan , R. Contreras Ramos , B. J. Pritzl , H. A. Smith , J. Alonso-Garcia

We present results of a search for variable stars in the intermediate-age open cluster NGC 7044. We found 23 variable stars in the observed field. One star turned out to be of the delta Sct type with two pulsational modes excited. From the…

太阳与恒星天体物理 · 物理学 2012-11-20 G. Kopacki , D. Drobek , Z. Kolaczkowski , G. Polubek

We present a short progress report of a comprehensive search for variability in the globular cluster 47 Tucanae. Using the MSSSO 40'' telescope and a combined V+R filter, we are searching for variability across a 52x52' field centered on…

天体物理学 · 物理学 2007-05-23 David T. F Weldrake , Penny D Sackett , Terry J Bridges

We obtained a series of more than two hundred R-band CCD images for the crowded central (115"x77") region of the metal-poor globular cluster M15 with an angular resolution of 0.5"-0.9" in most images. Optimal image subtraction was used to…

天体物理学 · 物理学 2009-11-10 Alexander P. Zheleznyak , Valery V. Kravtsov