Eclipsing binary stars in the Large Magellanic Cloud. Results from the EROS-2, OGLE and VMC surveys
arXiv:1406.2494 · doi:10.1093/mnras/stu1151
Abstract
We present a catalogue of 1768 eclipsing binary stars (EBs) detected in the Large Magellanic Cloud (LMC) by the second generation of the EROS survey (hereinafter EROS-2); 493 of them are new discoveries located in outer regions (out of the central bar) of the LMC. These sources were originally included in a list of candidate classical Cepheids (CCs) extracted from the EROS-2 catalogue on the basis of the period (0.89 15.85 days) versus luminosity ( mag) diagram. After visual inspection of the light curves we reclassified them as eclipsing binaries. They have blue colours ( 0.2 mag) hence we classed them as hot eclipsing binaries (HEBs) containing hot massive components: main sequence (MS) stars or blue giants. We present -band light curves for 999 binaries from our sample that have a counterpart in the VISTA near-infrared ESO public survey of the Magellanic Clouds system (VMC). We provide spectral classifications of 13 HEBs with existing spectroscopy. We divided our sample into contact-like binaries and detached/semi-detached systems based on both visual inspection and the parameters of the Fourier decomposition of the light curves and analysed the period-luminosity () relations of the contact-like systems using the and magnitudes at maximum light. The contact-like binaries in our sample do not follow relations. We analysed the sample of contact binaries from the OGLE III catalogue and confirmed that and sequences are defined only by eclipsing binaries containing a red giant component.
17 pages, 17 figures, 6 tables, accepted for publication in MNRAS
References in corpus (10)
- Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds
- An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent
- The VLT-FLAMES survey of massive stars: constraints on stellar evolution from the chemical compositions of rapidly rotating Galactic and Magellanic Cloud B-type stars
- The VLT-FLAMES Survey of Massive Stars: Observations centered on the Magellanic Cloud clusters NGC 330, NGC 346, NGC 2004, and the N11 region
- The VISTA Science Archive
- The VLT-FLAMES survey of massive stars: atmospheric parameters and rotational velocity distributions for B-type stars in the Magellanic Clouds
- New Optical Reddening Maps of the Large and Small Magellanic Clouds
- Ellipsoidal Variability and Long Secondary Periods in MACHO Red Giant Stars
- Eclipsing binaries in the MACHO database: New periods and classifications for 3031 systems in the Large Magellanic Cloud
- The beat Cepheids in the Magellanic Clouds: an analysis from the EROS-2 database
Cited by in corpus (9)
- The VMC Survey. XXV. The 3D structure of the Small Magellanic Cloud from Classical Cepheids
- The VMC survey - XXVI. Structure of the Small Magellanic Cloud from RR Lyrae stars
- The B-type Binaries Characterisation Programme I. Orbital solutions for the 30 Doradus population
- The VMC Survey -- XLII. Near-infrared period-luminosity relations for RR Lyrae stars and the structure of the Large Magellanic Cloud
- Contact Binaries as Viable Distance Indicators: New, Competitive (V)JHKs Period-Luminosity Relations
- Flying far and fast: the distribution of distant hypervelocity star candidates from Gaia DR2 data
- Zwicky Transient Facility and Globular Clusters: the Period-Luminosity and Period-Luminosity-Color Relations for Late-Type Contact Binaries
- Towards early-type eclipsing binaries as extragalactic milestones: I. Physical parameters of OGLE-LMC-ECL-22270 and OGLE-LMC-ECL-06782
- New variable sources revealed by DECam toward the LMC: the first 15 deg2