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相关论文: New SX Phoenicis Variables in the Globular Cluster…

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We present preliminary results of the variability survey in the field of the glo bular cluster NGC 4833. We observed all 34 variable stars known in the cluster. In add ition, we have found two new SX Phoenicis stars, one new RR Lyrae star,…

星系天体物理 · 物理学 2015-06-18 Grzegorz Kopacki

Using V images taken in May and June 2012 with the SARA Consortium's 0.9-meter telescope located at Kitt Peak National Observatory, we searched for variable stars in the globular cluster M107 (NGC 6171). The search was accomplished using…

太阳与恒星天体物理 · 物理学 2013-01-25 Thayne A. McCombs , Erik D. Reinhart , Andrew N. Darragh , Elliott W. Johnson , Brian W. Murphy

Using the Southeastern Association for Research in Astronomy 0.6 meter telescope located at Cerro Tololo, we searched for variable stars in the southern globular cluster NGC 6584. We obtained images during 8 nights between 28 May and 6 July…

太阳与恒星天体物理 · 物理学 2012-07-17 Joseph M. Toddy , Elliott W. Johnson , Andrew N. Darragh , Brian W. Murphy

We report the discovery of two new variable stars in the metal-poor globular cluster NGC 288, found by means of time-series CCD photometry. We classified the new variables as SX Phoenicis due to their characteristic fundamental mode periods…

太阳与恒星天体物理 · 物理学 2015-03-18 E. Martinazzi , S. O. Kepler , J. E. S. Costa , A. Pieres , C. Bonatto , E. Bica , L. Fraga

We present new BV CCD photometry, light curves, and ephemerides for 9 previously known, 29 newly detected RR Lyrae variables and one newly detected variable of an unknown type in the globular cluster M75. The photometry used for the…

天体物理学 · 物理学 2009-11-07 T. M. Corwin , M. Catelan , H. A. Smith , J. Borissova , F. R. Ferraro , W. S. Raburn

We present results of a search for variable stars in a region of the globular cluster NGC 4147 based on photometric observations with 4k x 4k CCD imager mounted at the axial port of the recently installed 3.6 m Devasthal optical telescope…

We present the analysis of 26 nights of V and I time-series observations from 2011 and 2012 of the globular cluster M 30 (NGC 7099). We used our data to search for variable stars in this cluster and refine the periods of known variables; we…

We report on the discovery of eleven multimode SX Phoenicis--type blue stragglers in the field of the southern globular cluster NGC 3201. In these variables both radial and non-radial modes are excited. For three variables the derived…

天体物理学 · 物理学 2009-11-07 B. Mazur , W. Krzeminski , I. B. Thompson

We present the results of a commissioning campaign to observe Galactic globular clusters for the search of microlensing events. The central 10' X 10' region of the globular cluster NGC 5024 was monitored using the 2-m Himalayan Chandra…

星系天体物理 · 物理学 2015-05-28 M. Safonova , C. S. Stalin

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,…

太阳与恒星天体物理 · 物理学 2017-09-04 M. A. Yepez , A. Arellano Ferro , S. Muneer , Sunetra Giridhar

We present B, V and I CCD light curves for 101 variable stars belonging to the globular cluster NGC2419, 60 of which are new discoveries, based on datasets obtained at the TNG, SUBARU and HST telescopes. The sample includes 75 RR Lyrae…

太阳与恒星天体物理 · 物理学 2015-05-20 M. Di Criscienzo , C. Greco , V. Ripepi , G. Clementini , M. Dall' Ora , M. Marconi , I. Musella , L. Federici , L. Di Fabrizio

We have performed a photometric V, R, I CCD time-series analysis with a baseline of ~8 years of the outer-halo globular cluster NGC 7492 with the aim of searching for new variables and using these (and the previously known variables) to…

太阳与恒星天体物理 · 物理学 2015-06-16 R. Figuera Jaimes , A. Arellano Ferro , D. M. Bramich , Sunetra Giridhar , K. Kuppuswamy

Time series BVI photometry is presented for 16 short-period variables located in the central region of the globular cluster NGC 6397. The sample includes 9 newly detected variables. The light curve of cataclysmic variable CV6 shows…

天体物理学 · 物理学 2016-08-30 Janusz Kaluzny , Ian B. Thompson

We report CCD V and I time series photometry of the globular cluster NGC 5024 (M53). The technique of difference image analysis has been used which enables photometric precisions better than 10 mmag for stars brighter than V 18.5mag even in…

太阳与恒星天体物理 · 物理学 2015-05-28 A. Arellano Ferro , R. Figuera Jaimes , Sunetra Giridhar , D. M. Bramich , J. V. Hernandez Santisteban , K. Kuppuswamy

Through time-series CCD photometry of the metal-poor globular cluster M53, we have discovered eight new SX Phoenicis type stars (labeled from SXP1 to SXP8). All the new SX Phoenicis stars are located in the blue straggler star region of a…

天体物理学 · 物理学 2009-11-07 Young-Beom Jeon , Myung Gyoon Lee , Seung-Lee Kim , Ho Lee

We present new photometry and analysis of the twelve variable stars (nine RR Lyrae, three SX Phoenicis) belonging to the Sagittarius globular cluster Arp 2. Of the nine RR Lyrae stars in the cluster, eight are RRab and one is RRc. From the…

太阳与恒星天体物理 · 物理学 2019-05-01 Barton J. Pritzl , Thomas C. Gehrman , Ricardo Salinas , Márcio Catelan , Horace A. Smith , Jura Borissova

We conducted a variable star search on the metal-rich Galactic globular cluster NGC 6652 using archival Gemini-S/GMOS data. We report the discovery of nine new variable stars in the NGC 6652 field, of which we classify six as eclipsing…

太阳与恒星天体物理 · 物理学 2019-01-23 Ricardo Salinas , A. Katherina Vivas , Rodrigo Contreras Ramos

We describe here results of a photometric time-sequence survey of the globular cluster M3 (NGC 5272), in a search for contact and detached eclipsing binary stars. We have discovered only one likely eclipsing binary and one SX Phe type star…

天体物理学 · 物理学 2016-08-30 J. Kaluzny , R. W. Hilditch , C. Clement , S. M. Rucinski

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…

The first calibrated broadband BVI time-series photometry is presented for the variable stars in NGC 2808, with observations spanning a range of twenty-eight years. We have also redetermined the variability types and periods for the…

太阳与恒星天体物理 · 物理学 2015-06-12 Andrea Kunder , Peter B. Stetson , Marcio Catelan , Alistair R. Walker , Pia Amigo
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