eclipsing binaries
Finding exoplanets around eclipsing binaries: a feasibility study using Mt Kent & Moore Observatories
... exoplanets.org and planetquest.jpl.nasa.gov provide great examples). But these searches have previously focused on single star systems or those in widely separated binary systems. In order to provide a more complete ...
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K2 variable catalogue : variable stars and eclipsing binaries in K2 campaigns 1 and 0
... The K2 mission will be of great use to a wide range of as- tronomical research areas. Although the original Kepler space telescope was primarily aimed at the detection and study of ex- oplanets, its high precision ...
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Four colour photometry of eclipsing binaries XL, uvby light curves for the B type systems DW Carinae, BF Centauri, AC Velorum, and NSV 5783
... A detailed analysis of DW Car, based on the new uvby light curves and 29 high-resolution spectra obtained with the FEROS spectrograph at the ESO 1.52 m telescope (Kaufer et al. 1999, 2000) is published separately ...
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Ten eclipsing binaries in the Small Magellanic Cloud: fundamental parameters and Cloud distance
... 100 eclipsing binaries in the Small Magellanic Cloud ...early-B binaries, six are in a semi-detached configu- ration, and one is in a marginal contact ...
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Photometric Study of Three Short Period Eclipsing Binaries from the ASAS Catalogue
... We present the results of our study of three previously unstudied short-period eclipsing binaries, namely: ASAS 110609 − 2045.3, ASAS105331 − 7424.7, and ASAS 130057 + 2120.3. Using the visual (V)-band data ...
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The EBLM project I Physical and orbital parameters, including spin orbit angles, of two low mass eclipsing binaries on opposite sides of the brown dwarf limit
... discovered eclipsing binaries comprising F, G, K primaries with M dwarf ...dwarf eclipsing binaries promises large numbers of masses and radii of low-mass stars over the entire range of M ...
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The BEBOP radial velocity survey for circumbinary planets I Eight years of CORALIE observations of 47 single line eclipsing binaries and abundance constraints on the masses of circumbinary planets
... EBLM binaries were already known to exist in- side a triple star ...Kepler eclipsing binaries were done so without any a priori knowledge of a tertiary com- ...
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Absolute dimensions of eclipsing binaries XXVI, Setting a new standard : masses, radii, and abundances for the F type systems AD Bootis, VZ Hydrae, and WZ Ophiuchi
... We believe our study is among the most detailed carried out to date for main-sequence eclipsing binaries, and that it sets new standards for critical tests of stellar evolutionary models based on accurate ...
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The palomar transient factory orion project: eclipsing binaries and young stellar objects
... of eclipsing binary systems for yielding accurate measurements of fundamental stellar parameters, such as mass, radius, and effective temperature ratio, makes them useful for constraining stellar ...PMS ...
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K2 variable catalogue – II Machine learning classification of variable stars and eclipsing binaries in K2 fields 0–4
... The full range of features used is described in Table 2. These features are incorporated largely to separate out light curves which show purely noise, something which is generally uninformed by the SOM, as well as those ...
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Eclipsing binaries from the cstar project at Dome A, Antarctica
... In the past several years, the Antarctic plateau has attracted the attention of many astronomers. It is extremely cold and dry, and has continuous polar nights. Dome A is located at longitude 77 06 57 ¢ E, latitude ...
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Absolute dimensions of eclipsing binaries XXIV, The Be star system DW Carinae, a member of the open cluster Collinder 228
... The properties of DW Car can be used to infer the proper- ties of its parent cluster, Cr 228. The distance modulus of the dEB, calculated using the empirical bolometric corrections of Flower (1996), is 12.24 ± 0.12 mag, ...
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Eclipsing binaries observed with the WIRE satellite II, β Aurigae and non linear limb darkening in light curves
... The study of detached eclipsing binaries (dEBs) is our primary source of accurate physical properties of normal stars (Andersen 1991). By modelling their light curves and deriving radial veloc- ities of the ...
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Eclipsing binaries observed with the WIRE satellite I, Discovery and photometric analysis of the new bright A0 IV eclipsing binary ψ Centauri
... As can be seen from Table 2, the fractional radii of the com- ponent stars of ψ Cen are known to impressive random errors of 0.10% (primary star) and 0.15% (secondary), and all of the light curve parameters are extremely ...
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CCD TIMES OF MINIMA OF AINT ECLIPSING BINARIES IN
... = times of minima were obtained by superposition of two or more parts of light urve from di erent nights.; type err = the type of variable star given in GCVS is wrong, new details will b[r] ...
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PERIOD–AGE CORRELATIONS FOR ECLIPSING BINARIES IN STELLAR CLUSTERS
... and 56 binary stars (6 EB and 50 EW type) from 13 globular clusters in the Galaxy. We considered only binary stars that, based on the literature data, belong to the cluster. If for a given star there is more than one ...
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IBVS Volume 6001
... The minima times were computed with the Kwee – van Woerden method (Kwee & van Woerden, 1956). Two remarkable minima observations are plotted in Figs. 1 and 2 below. The system V760 Oph shows one of the deepest ...
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The Gaia DR1 mass–radius relation for white dwarfs
... for eclipsing binaries strongly suggest that theoretical MRRs are in agreement with ...from eclipsing binaries may provide the key to disentangle a gen- uine observed signature of the white ...
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Kepler-10c: a 2.2 earth radius transiting planet in a multiple system
... foreground eclipsing binaries blended with the target as well as eclipsing binaries physically associated with the target in a hierarchical triple ...the eclipsing pair diluted by the ...
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14 new eclipsing white dwarf plus main-sequence binaries from the SDSS and Catalina surveys
... new eclipsing white dwarf plus main-sequence (WDMS) bi- naries in the light curves of the Catalina ...17 eclipsing systems, 14 of which are new ...candidate eclipsing systems, 2 main-sequence ...
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