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相关论文: Periodic Variables in the Open Cluster NGC 2301

200 篇论文

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

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…

天体物理学 · 物理学 2009-11-06 L. L. Kiss , Gy. Szabo , K. Sziladi , G. Furesz , K. Sarneczky , B. Csak

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

We have monitored a 3 deg2 area toward Serpens Main in the Pan-STARRS1 r, i, and z bands from 2016 April to September. Light curves of more than 11,000 stars in each band were obtained, and 143 variables have been identified. Among those,…

太阳与恒星天体物理 · 物理学 2021-07-14 Jia Yin , Zhiwei Chen , Rolf Chini , Martin Haas , Sadegh Noroozi , Yongqiang Yao , Zhibo Jiang , Xuan Qian , Liyong Liu , Yao Li

We present new discoveries of variable stars near the turnoff of the old open cluster NGC 7142. Contrary to previous studies, we detect eight contact or near contact eclipsing binaries (including three near the cluster turnoff), and most of…

太阳与恒星天体物理 · 物理学 2015-05-30 Eric L. Sandquist , Andrew W. Serio , Matthew Shetrone

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

Five fields located close to the center of the globular cluster NGC 104=47 Tuc were surveyed in a search for variable stars. We present V-band light curves for 42 variables. This sample includes 13 RR Lyr stars -- 12 of them belong to the…

天体物理学 · 物理学 2016-08-30 J. Kaluzny , M. Kubiak , M. Szymanski , A. Udalski , W. Krzeminski , M. Mateo , K. Stanek

The $13.6\times 13.6$ arcmin$^{2}$ field covering the central part of the globular cluster NGC~6397 was surveyed in a search for short-period variable stars. We obtained light curves for 6 close binaries, 2 SX~Phe stars and 1 RR~Lyrae…

天体物理学 · 物理学 2009-10-28 J. Kaluzny

We present time series photometry of 57 variable stars in the cluster region NGC 7380. The association of these variable stars to the cluster NGC 7380 has been established on the basis of two colour diagrams and colour-magnitude diagrams.…

太阳与恒星天体物理 · 物理学 2016-01-27 Sneh Lata , A. K. Pandey , Neelam Panwar , W. P. Chen , M. R. Samal , J. C. Pandey

We present a comprehensive re-analysis of stellar photometric variability in the field of the open cluster M37 following the application of a new photometry and de-trending method to MMT/Megacam image archive. This new analysis allows a…

太阳与恒星天体物理 · 物理学 2015-05-19 S. -W. Chang , Y. -I. Byun , J. D. Hartman

We have performed a search for variable stars in the dwarf irregular galaxy NGC 6822 using wide-field multi-epoch VI photometry down to a limiting magnitude $V$ $\sim$ 22. Apart from the Cepheid variables in this galaxy already reported in…

天体物理学 · 物理学 2009-11-11 R. E. Mennickent , W. Gieren , I. Soszynski , G. Pietrzynski

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 study photometric variability among the optical counterparts of X-ray sources in the old open cluster M67. The two puzzling binaries below the giant branch are both variables: for S1113 the photometric period is compatible with the…

天体物理学 · 物理学 2009-11-07 Maureen van den Berg , Keivan Stassun , Frank Verbunt , Robert D. Mathieu

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

We present time-series photometry of stars located in the extremely young open cluster Berkeley 59. Using the 1.04 m telescope at ARIES, Nainital, we have identified 42 variables in a field of 13'x13' around the cluster. The probable…

太阳与恒星天体物理 · 物理学 2015-05-30 Sneh Lata , A. K. Pandey , Maheswar G. , Soumen Mondal , Brijesh Kumar

We present time series data on the variable stars of the galactic globular cluster Messier 3 (M3). We give BVI light curves for 226 RR Lyrae, 2 SX Phe and 1 W Vir type variables, along with estimated fundamental photometric parameters such…

天体物理学 · 物理学 2009-11-11 J. M. Benko , G. A. Bakos , J. Nuspl

We describe the results of a search for transit-like events caused by giant planets occulting stars in the old, metal-rich open cluster NGC 6791 based on BVI-colour photometry from eight nights of observations with the 2.54m Nordic Optical…

天体物理学 · 物理学 2009-11-10 H. Bruntt , F. Grundahl , B. Tingley , S. Frandsen , P. B. Stetson , B. Thomsen

We present the list of variable stars we found in the \kep\ superstamp data covering approximately nine arcminutes from the central region of NGC6819. This is a continuation of our work presented by Sanjayan et al.(2022a). We classified the…

太阳与恒星天体物理 · 物理学 2024-05-08 S. Sanjayan , A. S. Baran , P. Nemeth , K. Kinemuchi

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…