{ "id": "1311.2818", "version": "v1", "published": "2013-11-12T15:46:46.000Z", "updated": "2013-11-12T15:46:46.000Z", "title": "Interpretation of the oscillation spectrum of HD 50230 - a failure of richness", "authors": [ "Wojciech Szewczuk", "Jadwiga DaszyƄska-Daszkiewicz", "Wojciech Dziembowski" ], "comment": "Proceedings IAU Symposium No. 301", "categories": [ "astro-ph.SR" ], "abstract": "Attempts to interpret the observed oscillation spectrum of the SPB star HD 50230 are reported. We argue that a nearly equidistant period spacing found in the oscillation spectrum of the star is most likely accidental. The observed period distribution requires excitation of modes with the degree $\\ell>4$. Much more may be learned from the rich oscillation spectrum of the star but most of the work is still ahead of us.", "revisions": [ { "version": "v1", "updated": "2013-11-12T15:46:46.000Z" } ], "analyses": { "keywords": [ "interpretation", "spb star hd", "rich oscillation spectrum", "period distribution", "equidistant period spacing" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2014IAUS..301..109S" } } }