{
  "id": "1411.1914",
  "version": "v1",
  "published": "2014-11-07T13:52:49.000Z",
  "updated": "2014-11-07T13:52:49.000Z",
  "title": "Connection between the period and the amplitude of the Blazhko effect",
  "authors": [
    "J. M. Benkő",
    "R. Szabó"
  ],
  "comment": "CoRoT Symposium 3 / Kepler KASC-7 joint meeting, Toulouse, July 2014. To be published by EPJ Web of Conferences",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We found a possible relationship between the modulation period and the amplitude of the Blazhko RR Lyrae stars: long modulation period generally implies high modulation amplitude while the short modulation period results in small amplitude. Although this effect is much more a tendency than a strict rule, it can be detected easily in the space-born time series data produced by Kepler and CoRoT. Good quality ground-based data show this relation, too. This phenomenon could give us constraints for the physics of the Blazhko effect.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2014-11-07T13:52:49.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "blazhko effect",
      "short modulation period results",
      "blazhko rr lyrae stars",
      "space-born time series data"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "adsabs": "2015EPJWC.10106008B"
    }
  }
}