J/AcA/56/219        OGLE variable stars in NGC 6259        (Ciechanowska+, 2006)

The Optical Gravitational Lensing Experiment. Variable stars in the field of open cluster NGC 6259. Ciechanowska A., Pietrzynski G., Wyrzykowski L., Szewczyk O., Kubiak M., Udalski A., Szymanski M.K. <Acta Astron., 56, 219-236 (2006)> =2006AcA....56..219C 2006AcA....56..219C (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, open ; Stars, variable ; Magnitudes Keywords: binaries: eclipsing - stars: oscillations - open clusters and associations: individual: NGC 6259 Abstract: We present the results of a search for variable stars in the field of NGC6259. Altogether 85 variable stars have been discovered. 36 of them are eclipsing systems. This group contains 13 EA, 2 EB and 21 EW-type stars. Light curves of two variable stars resemble those of Miras. The remaining 47 variable stars detected in the field of this open cluster are most probably highly obscured red giants (OSARG, irregular). For all detected variable stars we provide their light curves, preliminary classification, discussion on the possible cluster membership, equatorial coordinates, finding charts and periods when possible. Description: The presented data were collected from July 1997 to September 1999 during 44 nights in the course of the OGLE project (Udalski, Kubiak and Szymanski, 1997AcA....47..319U 1997AcA....47..319U) at the time, when the weather conditions were too poor to observe the very dense OGLE fields. All observations were made with 1.3m Warsaw telescope located at the Las Campanas Observatory, Chile which is operated by the Carnegie Institution of Washington. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 86 36 Eclipsing variable stars in NGC 6259 table4.dat 77 49 Miscellaneous variable stars in NGC 6259 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- VName Variable name (V1-V36) 5- 6 I2 h RAh Right ascension (J2000) 8- 9 I2 min RAm Right ascension (J2000) 11- 15 F5.2 s RAs Right ascension (J2000) 17 A1 --- DE- Declination sign (J2000) 18- 19 I2 deg DEd Declination (J2000) 21- 22 I2 arcmin DEm Declination (J2000) 24- 27 F4.1 arcsec DEs Declination (J2000) 29- 34 F6.3 mag Vmag ?=- V magnitude 36- 40 F5.3 mag e_Vmag ?=- rms uncertainty on Vmag 42- 47 F6.3 mag Imag I magnitude 49- 53 F5.3 mag e_Imag rms uncertainty on Imag 55- 59 F5.3 mag V-I ?=- V-I colour index 61- 66 F6.4 d Per ?=- Period 68- 73 F6.4 --- Phase ?=- Phase 75- 83 F9.4 d t0 ?=- Time of maximum brightness (HJD-2350000) 85- 86 A2 --- Type Type of eclipsing binary -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- VName Variable name (V37-V85) 5- 6 I2 h RAh Right ascension (J2000) 8- 9 I2 min RAm Right ascension (J2000) 11- 15 F5.2 s RAs Right ascension (J2000) 17 A1 --- DE- Declination sign (J2000) 18- 19 I2 deg DEd Declination (J2000) 21- 22 I2 arcmin DEm Declination (J2000) 24- 27 F4.1 arcsec DEs Declination (J2000) 29- 34 F6.3 mag Vmag ?=- V magnitude 36- 40 F5.3 mag e_Vmag ?=- rms uncertainty on Vmag 42- 47 F6.3 mag Imag ?=- I magnitude 49- 53 F5.3 mag e_Imag ?=- rms uncertainty on Imag 55- 59 F5.3 mag V-I ?=- V-I colour index 61- 77 A17 --- Type Variable type -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 17-May-2016
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line