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Find link is a tool written by Edward Betts.searching for Colliding-wind binary 12 found (24 total)
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NGC 6604
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of the most luminous stars in the galaxy. HD 168112 is another colliding-wind binary in the cluster; both systems are over-luminous in their X-ray emissionApep (star system) (3,237 words) [view diff] exact match in snippet view article
Molonglo Observatory Synthesis Telescope, and was noted as a potential colliding-wind binary, with a radio source as bright as Eta Carinae. Callingham and PeterWR 69 (568 words) [view diff] case mismatch in snippet view article find links to article
amplitude of 0.044 magnitudes, suggesting it could be a short period Colliding-Wind Binary. However, this period is not in fact due to binary, but due to theCygnus OB2-8A (671 words) [view diff] no match in snippet view article find links to article
R.; Van Loo, S. (2006). "XMM-Newton observations of the massive colliding wind binary and non-thermal radio emitter CygOB2#8A [O6If + O5.5III(f)]" (PDF)WR 25 (1,290 words) [view diff] exact match in snippet view article find links to article
Solivella, G. (2006). "The first orbital solution for the massive colliding-wind binary HD 93162 (≡WR 25)". Astronomy and Astrophysics. 460 (3): 777–782HD 93129 (1,195 words) [view diff] exact match in snippet view article find links to article
(2016). "A model for the non-thermal emission of the very massive colliding-wind binary HD 93129A". Astronomy & Astrophysics. 591: A139. arXiv:1604.07294WR 147 (1,294 words) [view diff] exact match in snippet view article find links to article
leading to a separation of about 0.33 AU. WR 140, the prototype colliding-wind binary Roman, Nancy G. (1987). "Identification of a constellation fromWR 133 (825 words) [view diff] exact match in snippet view article find links to article
M.; Schanne, L.; et al. (2011). "Spectroscopy of the archetype colliding-wind binary WR 140 during the 2009 January periastron passage". Monthly NoticesCygnus OB2 (1,717 words) [view diff] no match in snippet view article find links to article
R.; Van Loo, S. (2006). "XMM-Newton observations of the massive colliding wind binary and non-thermal radio emitter CygOB2#8A [O6If + O5.5III(f)]" (PDF)List of most luminous stars (10,664 words) [view diff] no match in snippet view article find links to article
High-resolution X-Ray Spectroscopy Suggests That Cyg OB2 12 is a Colliding Wind Binary". The Astrophysical Journal. 845 (1): 39. arXiv:1707.04473. Bibcode:2017ApJList of most massive stars (9,043 words) [view diff] exact match in snippet view article find links to article
(2025-03-21). "Melnick 39 is a very massive intermediate-period colliding-wind binary". arXiv:2503.17150. Wu, Shi-Wei; Bik, Arjan; Bestenlehner, JoachimWolf–Rayet star (10,616 words) [view diff] exact match in snippet view article find links to article
Bolingbroke, N.J. (2005). "High-resolution radio observations of the colliding-wind binary WR 140". The Astrophysical Journal. 623 (1): 447–459. arXiv:astro-ph/0501391