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相关论文: Variable Yellow and Red Stragglers in the Old Open…

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Time-series CCD photometric observations of the intermediate-age open cluster NGC 2099 were performed to search for variable stars. We also carried out BV photometry to study physical properties of variables in the cluster. Using V-band…

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

We studied solar-like oscillations in 115 red giants in the three open clusters NGC 6791, NGC 6811, and NGC 6819, based on photometric data covering more than 19 months with NASA's Kepler space telescope. We present the asteroseismic…

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 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

NGC 6791 is one of the richest old open clusters in the Milky Way. Its position above the Galactic plane and the number density makes it an interesting middle ground between Galactic open and globular clusters. We aim to detect the UV…

太阳与恒星天体物理 · 物理学 2023-08-09 Vikrant V. Jadhav , Annapurni Subramaniam , Ram Sagar

This work presents the first long-term photometric variability survey of the intermediate-age open cluster NGC 559. Time-series V band photometric observations on 40 nights taken over more than three years with three different telescopes…

太阳与恒星天体物理 · 物理学 2020-09-30 Yogesh C. Joshi , Ancy Anna John , Jayanand Maurya , Alaxendra Panchal , Brijesh Kumar , Santosh Joshi

The field of the globular cluster M12 (NGC 6218) was monitored between 1995 and 2009 in a search for variable stars. $BV$ light curves were obtained for 36 periodic or likely periodic variables. Thirty-four of these are new detections.…

太阳与恒星天体物理 · 物理学 2015-09-11 J. Kaluzny , I. B. Thompson , W. Narloch , W. Pych , M. Rozyczka

Three new photometric CCD-based datasets are presented for NGC~6791. They consist of deep UBV photometry (to $V_{lim} =24$, $B_{lim}=24$, $U_{lim} = 23$) of the central parts of the cluster and of selected fields around it, and of…

天体物理学 · 物理学 2016-08-30 Janusz Kaluzny , Slavek Rucinski

We report time-series photometry for 55 variable stars located in the central part of the globular cluster M55. The sample includes 28 newly identified objects of which 13 are eclipsing binaries. Three of these are detached systems located…

太阳与恒星天体物理 · 物理学 2010-11-04 J. Kaluzny , I. B. Thompson , W. Krzeminski , K. Zloczewski

We introduce the stellar sample of the WIYN Open Cluster Study radial-velocity survey for the rich open cluster NGC 7789 (1.6 Gyr, [Fe/H] = +0.02). This sample lies within an 18$'$ circular radius from the cluster center (10 pc in…

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…

太阳与恒星天体物理 · 物理学 2013-07-15 J. Kaluzny , I. B. Thompson , M. Rozyczka , W. Krzeminski

The field of the globular cluster NGC 3201 was monitored between 1998 and 2009 in a search for variable stars. $BV$ light curves were obtained for 152 periodic or likely periodic variables, 57 of which are new detections. Thirty-seven newly…

太阳与恒星天体物理 · 物理学 2016-10-10 J. Kaluzny , M. Rozyczka , I. B. Thompson , W. Narloch , B. Mazur , W. Pych , A. Schwarzenberg-Czerny

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

Context. Stars that are members of stellar clusters are assumed to be formed at the same time and place from material with the same initial chemical composition. These additional constraints on the ensemble of cluster stars make these stars…

太阳与恒星天体物理 · 物理学 2023-11-29 A. Covelo-Paz , N. Themeßl , F. Espinoza-Rojas , S. Hekker

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

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 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

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

(Abridged) We present results from 13776 radial-velocity (RV) measurements of 1278 candidate members of the old (4 Gyr) open cluster M67 (NGC 2682). The measurements are the results of a long-term survey that includes data from seven…

太阳与恒星天体物理 · 物理学 2015-09-16 Aaron M. Geller , David W. Latham , Robert D. Mathieu

BV photometry is presented for 12 RR Lyr variables discovered in the presumably young galactic globular cluster Ruprecht 106. All variables are type RRab, and their periods span a narrow range from 0.574 to 0.652 day. We report also on the…

天体物理学 · 物理学 2009-10-28 Janusz Kaluzny , Wojciech Krzeminski , Beata Mazur