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Latest comment: 7 months ago by Praemonitus in topic Probable triple star system
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Probable triple star system

[edit]

The following reference lists this as a "probable triple star" system with the third component being a dwarf of class K2:

Daszyńska-Daszkiewicz, J.; et al. (September 2017), Zwintz, Konnstanze; Poretti, Ennio (eds.), "The solitary g-mode frequencies in early B-type stars", Second BRITE-Constellation Science Conference: Small satellites—big science, Proceedings of the Polish Astronomical Society volume 5, held 22-26 August, 2016 in Innsbruck, Austria, Warsaw, Poland: Polish Astronomical Society, Bartycka 18, 00-716, pp. 138–144, arXiv:1701.00961, Bibcode:2017sbcs.conf..138D, doi:10.48550/arXiv.1701.00961.

Praemonitus (talk) 16:02, 14 December 2025 (UTC)Reply

I see this has been addressed. Thank you. Praemonitus (talk) 14:46, 15 December 2025 (UTC)Reply