WebThe Cygnus OB2 Association contains some of the most luminous OB stars in our Galaxy, the brightest of which are also among the most luminous in X-rays. WebBD+40° 4210 is a hot luminous giant star located in the constellation Cygnus. It is a member of the Cygnus OB2 association and a candidate Luminous Blue Variable. …
A spectroscopic study of the non-thermal radio emitter Cyg OB2 #8A ...
WebThere are several well-studied binary systems in Cyg OB2 whose radio emission appears as a single resolved source at ~150 mas resolution, that are detected with COBRaS. These include the 21.908±0.040 day, O6If + O5.5III binary Cyg OB2 #8A, which shows orbital phase-locked radio A&A, 519, 111). The resolution of e-MERLIN also allows a more … WebJul 23, 2024 · In this composite image of Cygnus OB2, X-rays from Chandra (red diffuse emission and blue point sources) are shown with optical data from the Isaac Newton Telescope (diffuse emission in light … bjorn wiinblad pottery
Cygnus OB2-8A Wiki
WebCygnus OA-8E. OA-8E was the ninth flight of the Orbital ATK uncrewed resupply spacecraft Cygnus and its eighth flight to the International Space Station (ISS) under the … Until 1951 Cyg OB2 #8 had been known only as an anonymous catalogue entry in the Bonner Durchmusterung. Then it was identified as one of several highly luminous hot stars close together in Cygnus. Despite being commonly referred to as Schulte #8A, the number 8 was first published in an earlier paper. Schulte … See more Cygnus OB2 #8A is a double-lined spectroscopic binary located near the centre of the Cygnus OB2 association located 5,500 light years away. See more • Cygnus OB2-8A on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images See more The Cygnus OB2 #8A system contains two massive luminous O class stars in a 21.9 day orbit. The primary is a 44 M☉ supergiant and the secondary is a 37 M☉ giant star. … See more WebWe present the results of a spectroscopic campaign revealing that the non-thermal radio emitter Cyg OB2 #8A is an O6 + O5.5 binary system. We propose the very first orbital solution indicating a period of about 21.9 days. The system appears to be eccentric (0.24 ± 0.04) and is likely seen under a rather low inclination angle. The mass ratio of the … bjorn willems