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Radial Velocity Monitoring Of (Candidate) Hybrid A- And F-Type Stars From The Kepler Mission

Authors: Lampens, Patricia; Vermeylen, Lore; De Cat, Peter; Sódor, Ádam; Bognár, Zsofia; Frémat, Yves; Skarka, Marek; +1 Authors

Radial Velocity Monitoring Of (Candidate) Hybrid A- And F-Type Stars From The Kepler Mission

Abstract

{"references": ["Balona, L. A. 2018, MNRAS, 476, 4840", "Balona, L. A., Daszy\u0144ska-Daszkiewicz, J., & Pamyatnykh, A. A. 2015, MNRAS, 452, 3073", "Grigahc\u00e8ne, A., Antoci, V., Balona, L., Catanzaro, G., Daszy\u0144ska-Daszkiewicz, J., et al. 2010, ApJ, 713, L192", "Irwin, J. B. 1952, ApJ, 116, 211", "Koubsk\u00fd, P., Mayer, P., \u010c\u00e1p, J., \u017d\u010f\u00e1rsk\u00fd, F., Zeman, J., et al. 2004, Publications of the Astronomical Institute of the Czechoslovak Academy of Sciences, 92, 37", "Lampens, P., Fr\u00e9mat, Y., Vermeylen, L., S\u00f3dor, \u00c1., Skarka, M., et al. 2018, A&A, 610, A17", "Murphy, S. J. & Shibahashi, H. 2015, MNRAS, 450, 4475", "Nemec, J. M., Balona, L. A., Murphy, S. J., Kinemuchi, K., & Jeon, Y.-B. 2017, MNRAS, 466, 1290", "Raskin, G., van Winckel, H., Hensberge, H., Jorissen, A., Lehmann, H., et al. 2011, A&A, 526, A69", "Reyniers, K. & Smeyers, P. 2003, A&A, 404, 1051", "Shibahashi, H., Murphy, S. J., & Kurtz, D. W. 2016, IAU Focus Meeting, 29, 642", "Uytterhoeven, K., Moya, A., Grigahc\u00e8ne, A., Guzik, J. A., Guti\u00e9rrez-Soto, J., et al. 2011, A&A, 534, A125"]}

An ensemble of 50 candidate hybrid A/F-type stars from the Kepler mission was monitored during four years with the HERMES spectrograph attached to the Mercator telescope. From this survey, we obtained new radial velocities, new or improved atmospheric properties (Teff, log g, v sin i), and classified all our targets in terms of evidence for multiplicity, pulsation and/or fast rotation. An extension of 40 new candidate hybrid A- and F-type stars from the Kepler mission has been recently defined for a second survey to be performed under similar conditions. The new high-resolution spectra will be obtained with various small and medium-sized telescopes. For a number of newly detected stellar systems with good radial velocity coverage, we also computed much improved orbits by combining the radial velocities with the time delays obtained via the monitoring of the pulsation frequencies during the four years of Kepler photometry.

Keywords

technique: radial velocity - stars: oscillations - stars: binary systems - stars: multiple systems - fundamental stellar parameters, Spectroscopy - radial velocities - A- and F-type stars - hybrid pulsating stars - stellar systems - Kepler mission, Spectroscopy - radial velocities - A- and F-type stars - hybrid pulsating stars - stellar systems - Kepler mission

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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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