J/A+A/640/A33   LMC 162 eccentric eclipsing binaries light curve (Zasche+, 2020)

First apsidal motion and light curve analysis of 162 eccentric eclipsing binaries from LMC. Zasche P., Wolf M., Kucakova H., Kara J., Merc J., Zejda M., Skarka M., Janik J., Kurfurst P. <Astron. Astrophys. 640, A33 (2020)> =2020A&A...640A..33Z 2020A&A...640A..33Z (SIMBAD/NED BibCode)
ADC_Keywords: Magellanic Clouds ; Binaries, eclipsing ; Photometry Keywords: binaries: eclipsing - stars: fundamental parameters - stars: early-type - Magellanic Clouds Abstract: We present an extensive study of 162 early-type binary systems located in the LMC galaxy that show apsidal motion and have never been studied before. For the ample systems, we performed light curve and apsidal motion modelling for the first time. These systems have a median orbital period of 2.2 days and typical periods of the apsidal motion were derived to be of the order of decades. We identified two record-breaking systems. The first, OGLE LMC-ECL-22613, shows the shortest known apsidal motion period among systems with main sequence components (6.6 years); it contains a third component with an orbital period of 23 years. The second, OGLE LMC-ECL-17226, is an eccentric system with the shortest known orbital period (0.9879 days) and with quite fast apsidal motion period (11 years). Among the studied systems, 36 new triple-star candidates were identified based on the additional period variations. This represents more than 20% of all studied systems, which is in agreement with the statistics of multiples in our Galaxy. However, the fraction should only be considered as a lower limit of these early-type stars in the LMC because of our method of detection, data coverage, and limited precision of individual times of eclipses. Description: For our whole analysis we only used the photometric data. Databases like OGLE and MACHO were used when available, while for some systems new photometry from the Danish 1.54 m telescope (hereafter DK154) was also obtained. The Photometric data from Danish 1.54-m telescope are presented. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file stars.dat 73 56 List of studied stars table.dat 39 26929 Photometric data from Danish 1.54-m telescope for 162 eccentric eclipsing binaries from LMC -------------------------------------------------------------------------------- See also: J/AcA/66/421 : Eclipsing binaries in the Magellanic System (Pawlak+, 2016) Byte-by-byte Description of file: stars.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 A19 --- Star Name of the star, OGLE LMC-ECL-NNNNN 20- 21 I2 h RAh Simbad Right Ascension (J2000.0) 23- 24 I2 min RAm Simbad Right Ascension (J2000.0) 26- 30 F5.2 s RAs Simbad Right Ascension (J2000.0) 32 A1 --- DE- Simbad Declination sign (J2000.0) 33- 34 I2 deg DEd Simbad Declination (J2000.0) 36- 37 I2 arcmin DEm Simbad Declination (J2000.0) 39- 42 F4.1 arcsec DEs Simbad Declination (J2000.0) 44- 52 F9.7 d Per Period (from table A2) 55- 63 F9.7 d e_Per rms uncertainty on Per (from table A2) 65- 68 I4 --- NR ? Number of measurements in R band 70- 73 I4 --- NI ? Number of measurements in I band -------------------------------------------------------------------------------- Byte-by-byte Description of file: table.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 A19 --- Star Name of the star, OGLE LMC-ECL-NNNNN 20- 30 F11.5 d HJD Heliocentric Julian Date (HJD-2400000) 32- 37 F6.3 mag mag Differential magnitude 39 A1 --- Filter [RI] Photometric filter used ------------------------------------------------------------------------------- Acknowledgements: Petr Zasche, zasche(at)sirrah.troja.mff.cuni.cz
(End) Patricia Vannier [CDS] 17-Jun-2020
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