The most massive heartbeat: an in-depth analysis of ι Orionis

Abstract ι Ori is a well-studied massive binary consisting of an O9 III + B1 III/IV star. Due to its high eccentricity (e = 0.764) and short orbital period (Porb = 29.133 76 d), it has been considered to be a good candidate to show evidence of tidal effects; however, none have previously been identi...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2017-05, Vol.467 (2), p.2494-2503
Hauptverfasser:	Pablo, Herbert, Richardson, N. D., Fuller, J., Rowe, J., Moffat, A. F. J., Kuschnig, R., Popowicz, A., Handler, G., Neiner, C., Pigulski, A., Wade, G. A., Weiss, W., Buysschaert, B., Ramiaramanantsoa, T., Bratcher, A. D., Gerhartz, C. J., Greco, J. J., Hardegree-Ullman, K., Lembryk, L., Oswald, W. L.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Physics Sciences of the Universe
Online-Zugang:	Volltext
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