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 … WebSep 16, 2024 · Article Contents ABSTRACT 1 INTRODUCTION 2 THE EXISTING OB ASSOCIATIONS IN CYGNUS 3 IDENTIFYING AND CHARACTERIZING OB STARS 4 IDENTIFYING NEW OB ASSOCIATIONS 5 ANALYSIS OF THE NEW OB ASSOCIATIONS 6 DISCUSSION 7 CONCLUSIONS ACKNOWLEDGEMENTS DATA AVAILABILITY …
Table 1. Parameters of Cyg OB2 No. 8A used in this work.
WebAims. Cyg OB2 #8A is a massive O-type binary displaying strong non-thermal radio emission. Owing to the compactness of this binary, emission of non-thermal X-ray … 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 … dick\\u0027s sporting goods gurnee
Wikizero - Cygnus OB2-8A
WebCygnus OB2 is a large young cluster of stars in the constellation of Cygnus.. The cluster is an OB association.It includes some of the most massive and most luminous stars known. … 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 … city bus 33 plymouth