315 research outputs found

    Seventy new non-eclipsing BEER binaries discovered in CoRoT lightcurves and confirmed by RVs from AAOmega

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    We applied the BEER algorithm to the CoRoT lightcurves from the first five LRc fields and identified 481481 non-eclipsing BEER candidates with periodic lightcurve modulations and amplitudes of 0.5870.5-87 mmag. Medium-resolution spectra of 281281 candidates were obtained in a seven-night AAOmega radial-velocity (RV) campaign, with a precision of 1\sim1 km/s. The RVs confirmed the binarity of 7070 of the BEER candidates, with periods of 0.3100.3-10 days.Comment: 2 pages, 1 figure, to appear in the CoRoT Symposium 3, Kepler KASC-7 joint meeting, EPJ Web of Conference

    BEER analysis of Kepler and CoRoT light curves. III. Spectroscopic confirmation of seventy new beaming binaries discovered in CoRoT light curves

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    (abridged for arXiv) The BEER algorithm searches stellar light curves for the BEaming, Ellipsoidal, and Reflection photometric modulations that are caused by a short-period companion. Applying the search to the first five long-run center CoRoT fields, we identified 481481 non-eclipsing candidates with periodic flux amplitudes of 0.5870.5-87 mmag. Optimizing the Anglo-Australian-Telescope pointing coordinates and the AAOmega fiber-allocations with dedicated softwares, we acquired six spectra for 231231 candidates and seven spectra for another 5050 candidates in a seven-night campaign. Analysis of the red-arm AAOmega spectra, which covered the range of 83428842A˚8342-8842\AA{}, yielded a radial-velocity precision of 1\sim1 km/s. Spectra containing lines of more than one star were analyzed with the two-dimensional correlation algorithm TODCOR. The measured radial velocities confirmed the binarity of seventy of the BEER candidates45-45 single-line binaries, 1818 double-line binaries, and 77 diluted binaries. We show that red giants introduce a major source of false candidates and demonstrate a way to improve BEER's performance in extracting higher fidelity samples from future searches of CoRoT light curves. The periods of the confirmed binaries span a range of 0.3100.3-10 days and show a rise in the number of binaries per Δ\DeltalogPP toward longer periods. The estimated mass ratios of the double-line binaries and the mass ratios assigned to the single-line binaries, assuming an isotropic inclination distribution, span a range of 0.0310.03-1. On the low-mass end, we have detected two brown-dwarf candidates on a 1\sim1 day period orbit. This is the first time non-eclipsing beaming binaries are detected in CoRoT data, and we estimate that 300\sim300 such binaries can be detected in the CoRoT long-run light curves.Comment: 28 pages, 15 figures, and 11 tables. Accepted for publication in A&

    Features of Gaia DR3 Spectroscopic Binaries I. Tidal circularization of Main-Sequence Stars

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    Previous studies pointed out that many observed samples of short-period binaries display a cutoff period, PcutP_{\rm cut}, such that almost all binaries with periods shorter than PcutP_{\rm cut} have circular orbits. This feature is probably due to long-term circularization processes induced by tidal interaction between the two stars of each binary. It seemed as if coeval main-sequence (MS) samples of open clusters display PcutP_{\rm cut} that depends on the sample age. Using the unprecedentedly large sample of MS spectroscopic orbits recently released by Gaia\textit{Gaia} we have found that the PcutP_{\rm cut} does not depend on the stellar age but, instead, varies with stellar temperature, decreasing linearly from 6.56.5 day at Teff5700T_{\rm eff}\sim 5700 K to 2.5\sim 2.5 day at 68006800 K. PcutP_{\rm cut} was derived by a new algorithm that relied on clear upper envelopes displayed in the period-eccentricity diagrams. Our PcutP_{\rm cut} determines both the border between the circular and eccentric binaries and the location of the upper envelope. The results are inconsistent with the theory which assumes circularization occurs during the stellar MS phase, a theory that was adopted by many studies. The circularization has probably taken place at the pre-main-sequence phase, as suggested already in 1989 by Zahn and Bouchet, and later by Khaluillin and Khaluillina in 2011. Our results suggest that the weak dependence of PcutP_{\rm cut} on the cluster age is not significant, and/or might be due to the different temperatures of the samples. If indeed true, this has far-reaching implications for the theory of binary and exoplanet circularization, synchronization, and alignment.Comment: 13 pages, 12 figures, 2 tables. Accepted for publication in MNRA

    An Experimental Investigation of Epistemic Modal Adverbs and Adjectives

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    This paper analyses epistemic modal adverbs and adjectives, both theoretically and experimentally, while addressing the prevalent conceptions of modality and context update. While modality is standardly viewed and represented uniformly, we show that epistemic modal adverbs and adjectives differ in various linguistic environments, and present experimental evidence that supports the claim that epistemic modal adverbs and adjectives differ in terms of cognitive processing. While context update is standardly viewed as a two-stage process composed of assertion and acceptance/rejection, we present experimental evidence that supports the claim that there is also a stage of evaluation, in which the hearer considers the content of the assertion and the implications of adding this content to the common ground
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