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Based on photometric data obtained between 1935 and 2017, $O-C$ diagrams were built for 22 RR Lyrae stars in the globular cluster NGC 6171, leading to the discovery of secular period changes in 4 variables for which we have calculated their…

Solar and Stellar Astrophysics · Physics 2018-06-13 A. Arellano Ferro , P. Rosenzweig , A. Luna , D. Deras , S. Muneer , S. Giridhar , R. Michel

A CCD photometric study of the dense galactic open cluster M37 is presented and discussed. The majority of the analysed data are time-series measurements obtained through an R_C filter. The observations were carried out on seven nights…

Astrophysics · Physics 2009-11-06 L. L. Kiss , Gy. Szabo , K. Sziladi , G. Furesz , K. Sarneczky , B. Csak

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…

Solar and Stellar Astrophysics · Physics 2012-11-20 G. Kopacki , D. Drobek , Z. Kolaczkowski , G. Polubek

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…

Solar and Stellar Astrophysics · Physics 2018-09-27 Fang-Fang Song , Ali Esamdin , Lu Ma , Jin-Zhong Liu , Yu Zhang , Hu-Biao Niu , Tao-Zhi Yang

We report the discovery of 6 SX Phoenicis stars in the southern globular cluster NGC 4833. Images were obtained from January through June 2011 with the Southeastern Association for Research in Astronomy 0.6 meter telescope located at Cerro…

Solar and Stellar Astrophysics · Physics 2012-07-17 Andrew N. Darragh , Brian W. Murphy

We present time-series VI photometry of the metal-rich globular cluster NGC 6316. Our color-magnitude diagrams show a predominantly red-clump horizontal branch morphology with no evidence of the blue extensions seen in NGC 6388 and NGC…

Astrophysics · Physics 2009-11-07 A. C. Layden , B. T. Bowes , D. L. Welch , T. M. A. Webb

The central part of the globular cluster NGC 288 was surveyed in a search for short-period variable stars. We obtained the V-band light curves for 4 SX Phe stars and 2 RR Lyrae variables, five of which are new discoveries. All SX Phe stars…

Astrophysics · Physics 2007-05-23 J. Kaluzny

We present the results of our search for variable stars in the intermediate-age open cluster NGC 7789. We have found 45 variable stars: 35 eclipsing binaries, five pulsating variables and five miscellaneous variables. Most of the eclipsing…

Astrophysics · Physics 2007-05-23 B. J. Mochejska , J. Kaluzny

We extract light curves for 4554 objects with $9<G<19$ in the K2 superstamp observations of the globular cluster M4, including 3784 cluster members, and search for variability. Among cluster member objects, we detect 66 variables, of which…

Solar and Stellar Astrophysics · Physics 2019-09-25 Joshua J. Wallace , Joel D. Hartman , Gaspar A. Bakos , Waqas Bhatti

We report time-series photometry for 16 variable stars located in the central part of the globular cluster NGC 6752. The sample includes 13 newly identified objects. The precision of our differential photometry ranges from 1 mmag at V=14.0…

Solar and Stellar Astrophysics · Physics 2014-11-20 Janusz Kaluzny , Ian B. Thompson

New accurate and homogeneous optical UBVRI photometry has been obtained for variable stars in the Galactic globular $\omega$ Cen (NGC 5139). We secured 8202 CCD images covering a time interval of 24 years and a sky area of 84x48 arcmin. The…

We have applied Alard's image subtraction method (ISIS v2.1) to the observations of the globular clusters NGC 6388 and NGC 6441 previously analyzed using standard photometric techniques (DAOPHOT, ALLFRAME). In this reanalysis of…

We have performed a careful investigation of the 74 candidate variable stars presented by Safanova & Stalin (2011). For this purpose we used our data base of imaging and light curves from Arellano Ferro et al. (2011) and Arellano Ferro et…

Solar and Stellar Astrophysics · Physics 2015-06-05 D. M. Bramich , A. Arellano Ferro , R. Figuera Jaimes , Sunetra Giridhar

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…

Astrophysics of Galaxies · Physics 2013-09-11 Devesh Path Sariya , Sneh Lata , R. K. S. Yadav

Our multi-epoch survey of ~20 sq. deg. of the Canis Major overdensity has detected only 10 RR Lyrae stars (RRLS). We show that this number is consistent with the number expected from the Galactic halo and thick disk populations alone,…

Astrophysics of Galaxies · Physics 2009-11-13 Cecilia Mateu , A. Katherina Vivas , Robert Zinn , Lissa Miller , Carlos Abad

We have performed the first study of the variable star population of Ursa Major I (UMa I), an ultra-faint dwarf satellite recently discovered around the Milky Way by the Sloan Digital Sky Survey. Combining time series observations in the B…

(Abridged) We present CCD BVI photometry of 85 variable stars from the field of the globular cluster NGC 6934. The photometry was obtained with the image subtraction package ISIS. 35 variables are new identifications: 24 RRab stars, 5 RRc…

Astrophysics · Physics 2009-10-31 J. Kaluzny , A. Olech , K. Z. Stanek

We present results of variability search in the field of the young open cluster NGC 1502. Eight variable stars were discovered. Of six other stars in the observed field that were suspected for variability, we confirm variability of two,…

Solar and Stellar Astrophysics · Physics 2009-12-04 G. Michalska , A. Pigulski , M. Stęślicki , A. Narwid

NGC 1851 is an intriguing Galactic globular cluster, with multiple stellar evolutionary sequences, light and heavy element abundance variations and indications of a surrounding stellar halo. We present the first results of a spectroscopic…

Solar and Stellar Astrophysics · Physics 2015-08-26 Colin A. Navin , Sarah L. Martell , Daniel B. Zucker

We use the fundamental-mode RR Lyr-type variable stars (RRab) from OGLE-IV survey to draw a 3D picture of the central part of the tidally disrupted Sagittarius Dwarf Spheroidal (Sgr dSph) galaxy. We estimate the line-of-sight thickness of…

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