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相关论文: Variability Study of EHB Stars in the Globular Clu…

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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…

太阳与恒星天体物理 · 物理学 2014-11-20 Janusz Kaluzny , Ian B. Thompson

We present the results of a photometric survey for variable stars in the field of the nearby globular cluster NGC 6752. The cluster was monitored in 1996 and 1997 for a total of 54 hours with 3 different CCD cameras mounted on the 1.0-m…

天体物理学 · 物理学 2009-10-31 Ian B. Thompson , Janusz Kaluzny , Wojtek Pych , Wojtek Krzeminski

We describe the status of a project whose main goal is to detect variability along the extreme horizontal branch of the globular cluster NGC 6752. Based on Magellan 6.5m data, preliminary light curves are presented for some candidate…

We have analyzed archival HST/WFPC2 time-series data of the central parts of globular clusters M13, M30 and NGC 6712 in search of variable objects. Among a total of 21 identified variables there are 15 new discoveries. The sample includes…

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

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 performed a spectroscopic search for binaries among hot Horizontal Branch stars in globular clusters. We present final results for a sample of 51 stars in NGC6752, and preliminary results for the first 15 stars analyzed in M80. The…

天体物理学 · 物理学 2007-05-23 C. Moni Bidin , R. A. Mendez , S. Moehler , G. Piotto , A. Recio-Blanco , Y. Momany

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,…

太阳与恒星天体物理 · 物理学 2009-12-04 G. Michalska , A. Pigulski , M. Stęślicki , A. Narwid

Aims: This work presents a high--precision variability survey in the field of the old, super metal-rich open cluster NGC 6791. Methods: The data sample consists of more than 75,000 high-precision CCD time series measurements in the V band…

We present the list of variable stars we found in the Kepler superstamp data covering approximately 9 arcminutes from the central region of NGC 6791. We classified the variable stars based on the variability type and we established their…

太阳与恒星天体物理 · 物理学 2023-03-15 Sachu Sanjayan , Andrzej S Baran , Peter Nemeth , Karen Kinemuchi , Jakub Ostrowski , Sumanta Kumar Sahoo

We have completely mapped the globular cluster NGC 1851 with VI CCD photometry, obtaining a CMD for ca. 20500 stars. From the apparent luminosity of the HB we derive a distance modulus (m-M)o=15.44+/-0.20. The presence of 7 "supra-HB" stars…

天体物理学 · 物理学 2007-05-23 I. Saviane , G. Piotto , F. Fagotto , S. Zaggia , M. Capaccioli , A. Aparicio

We present an analysis of $\emph{VI}$ CCD time series photometry of globular cluster NGC 6712. Our main goal is to study the variable star population as indicators of the cluster mean physical parameters. We employed the Fourier…

太阳与恒星天体物理 · 物理学 2020-01-29 D. Deras , A. Arellano Ferro , C. Lázaro , I. H. Bustos Fierro , J. H. Calderón , S. Muneer , S. Giridhar

V-band time-series CCD photometric observations of the intermediate-age open cluster M11 were performed to search for variable stars. Using these time-series data, we carefully examined light variations of all stars in the observing field.…

天体物理学 · 物理学 2009-11-13 J. -R. Koo , S. -L. Kim , S. -C. Rey , C. -U. Lee , Y. H. Kim , Y. B. Kang , Y. -B. Jeon

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…

太阳与恒星天体物理 · 物理学 2019-09-25 Joshua J. Wallace , Joel D. Hartman , Gaspar A. Bakos , Waqas Bhatti

We present spectroscopic analyses of 17 faint blue stars in the globular cluster NGC 6752. Effective temperatures, surface gravities, and helium abundances are determined and compared to theoretical predictions. All stars are helium…

天体物理学 · 物理学 2007-05-23 Sabine Moehler , Uli Heber , Gero Rupprecht

A photometric study of variable stars in the field of old open cluster NGC 188 is discussed. Observations were carried out in two bands R and I for 5513 stars up to R = 17 mag in the field of 1.5 x 1.5 grad. around the cluster. The…

太阳与恒星天体物理 · 物理学 2013-04-19 A. A. Popov , V. V. Krushinsky , E. A. Avvakumova , A. Y. Burdanov , A. F. Punanova , I. S. Zalozhnih

We report on the Chandra ACIS-S3 imaging observation of the globular cluster NGC 6752. We detect 6 X-ray sources within the 10.5" core radius and 13 more within the 115" half-mass radius down to a limiting luminosity of Lx approx 10^{30}…

We present the first results of our variability survey for the globular cluster NGC 362. We found numerous variable stars in the field including 23 RR Lyr stars, 4 eclipsing binaries and 5 other pulsating stars. Four of the RR Lyr ae stars…

天体物理学 · 物理学 2010-12-09 P. Székely , L. L. Kiss , B. Csák , A. Derekas , T. R. Bedding , K. Szatmáry

We present results of a UBVIc variability survey in the young open cluster NGC 2244. In total, we found 245 variable stars. Most of them, 211 stars, are variables with irregular variations. Furthermore, 23 periodic variables were found. We…

太阳与恒星天体物理 · 物理学 2019-06-12 Gabriela Michalska

The field of the globular cluster NGC 6362 was monitored between 1995 and 2009 in a search for variable stars. BV light curves were obtained for 69 periodic variables including 34 known RR Lyr stars, 10 known objects of other types and 25…

太阳与恒星天体物理 · 物理学 2015-01-22 J. Kaluzny , I. B. Thompson , M. Rozyczka , W. Pych , W. Narloch

Based on over 5400 BV images of 47 Tuc collected between 1998 and 2010 we obtained light curves of 65 variables, 21 of which are newly detected objects. New variables are located mostly just outside of the core in a region poorly studied by…

太阳与恒星天体物理 · 物理学 2014-05-26 J. Kaluzny , M. Rozyczka , W. Pych , W. Krzeminski , K. Zloczewski , W. Narloch
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