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Related papers: Variable stars in young open star cluster NGC 7380

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NGC 7129 is a bright reflection nebula located in the molecular cloud complex near l=105.4, b=+9.9, about 1.15 kpc distant. Embedded within the reflection nebula is a young cluster dominated by a compact grouping of four early-type stars:…

Solar and Stellar Astrophysics · Physics 2015-06-03 S. E. Dahm , L. A. Hillenbrand

Studying stellar pulsations in open clusters offers the possibility to perform ensemble asteroseismology. The reasonable assumption that the cluster members have the same age, distance, and overall metallicity aids in the seismic modelling…

Solar and Stellar Astrophysics · Physics 2015-05-28 G. Handler , S. Meingast

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…

Solar and Stellar Astrophysics · Physics 2014-05-26 J. Kaluzny , M. Rozyczka , W. Pych , W. Krzeminski , K. Zloczewski , W. Narloch

In this second paper on our variability survey of central stars of planetary nebulae (CSPNe) using ZTF, we report 11 long-timescale variables with variability timescales ranging from months to years. We also present preliminary analyses…

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 -…

Astrophysics · Physics 2009-06-25 M. Rozyczka , J. Kaluzny , W. Krzeminski , B. Mazur

We performed R-band time series observations of the young, metal rich open cluster NGC 2301 for 12 nights in Feb. 2004. B images were also obtained and color magnitude diagrams, having limits of R=19.5 and B=21.5, were produced. Only asmall…

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 a new search for variable stars in the Galactic globular cluster M28 (NGC 6626). The search is based on a series of BVI images obtained with the SMARTS Consortium's 1.3m telescope at Cerro Tololo Inter-American Observatory,…

Solar and Stellar Astrophysics · Physics 2015-06-05 G. Prieto , M. Catelan , R. Contreras Ramos , B. J. Pritzl , H. A. Smith , J. Alonso-Garcia

The extremely young cluster IC 348 has been monitored in the Cousins I band with a 0.6 m telescope at Wesleyan's Van Vleck Observatory. Photometry of 150 stars was obtained on 76 images taken on 27 separate nights during the period…

Astrophysics · Physics 2009-10-31 W. Herbst , J. A. Maley , E. C Williams

We present a spectroscopic analysis of the GIRAFFE and UVES data collected by the Gaia-ESO survey for the young open cluster NGC 3293. Archive spectra from the same instruments obtained in the framework of the `VLT-FLAMES survey of massive…

We present the results of a photometric survey for variable stars in the central region of the nearby globular cluster NGC 6397.Time series photometry was obtained for 30 variable objects. The sample includes 12 new objects, of which 6 show…

Astrophysics · Physics 2009-11-13 J. Kaluzny , I. B. Thompson , W. Krzeminski

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…

Solar and Stellar Astrophysics · Physics 2021-03-10 M. Rozyczka , W. Narloch , A. Schwarzenberg - Czerny , I. B. Thompson , R. Poleski , W. Pych

This is the second in a series of papers studying the variable stars in Large Magellanic Cloud globular clusters. The primary goal of this series is to study how RR Lyrae stars in Oosterhoff-intermediate systems compare to their…

Solar and Stellar Astrophysics · Physics 2015-06-11 Charles A. Kuehn , Horace A. Smith , Marcio Catelan , Barton J. Pritzl , Nathan De Lee , Jura Borissova

This paper reports results from our long-term $BV(RI)_{c}$ photometric CCD observations of eight pre-main-sequence stars collected from June 2008 to October 2022. These stars are located in the young open cluster Trumpler 37, in the field…

Solar and Stellar Astrophysics · Physics 2023-07-26 Sunay Ibryamov , Gabriela Zidarova , Evgeni Semkov , Stoyanka Peneva

We present simultaneous photometric and spectroscopic observations of seven young and highly variable M dwarfs in star forming regions in Orion, conducted in 4 observing nights with FORS2 at ESO/VLT. All seven targets show significant…

Solar and Stellar Astrophysics · Physics 2016-02-26 I. Bozhinova , A. Scholz , J. Eislöffel

We look for high-amplitude variable young stars in the open clusters and associations of the Orion Belt. We use public data from the ASAS-3 Photometric V-band Catalogue of the All Sky Automated Survey, infrared photometry from the 2MASS and…

Solar and Stellar Astrophysics · Physics 2015-05-14 Jose A. Caballero , M. Cornide , E. de Castro

Spectroscopy for 247 stars towards the young cluster NGC 346 in the Small Magellanic Cloud has been combined with that for 116 targets from the VLT-FLAMES Survey of Massive Stars. Spectral classification yields a sample of 47 O-type and 287…

Solar and Stellar Astrophysics · Physics 2019-06-19 P. L. Dufton , C. J. Evans , I. Hunter , D. J. Lennon , F. R. N. Schneider

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…

Solar and Stellar Astrophysics · Physics 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 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…

Astrophysics · Physics 2016-08-30 J. Kaluzny , R. W. Hilditch , C. Clement , S. M. Rucinski
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