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- Q22086962 subject Q7009396.
- Q22086962 subject Q7824699.
- Q22086962 subject Q8691170.
- Q22086962 abstract "UW Coronae Borealis, also known as MS1603.6+2600, is a low mass X-ray binary star system located in the constellation Corona Borealis. Astronomer Simon Morris and colleagues discovered the X-ray source in 1990 and were able to match it up with a faint star with an average visual magnitude of 19.4. The system is thought to be made up of a neutron star that has an accretion disk that draws material from its companion, a star less massive than the Sun. The disk is asymmetrical. The variability of the system is complex, with several periods identified: the two components orbit each other every 111 minutes, while there is another period of 112.6 minutes. The beat period of these is 5.5 days, which is thought to represent the precession of the asymmetrical accretion disk around the neutron star.".
- Q22086962 wikiPageWikiLink Q10406.
- Q22086962 wikiPageWikiLink Q237604.
- Q22086962 wikiPageWikiLink Q2703.
- Q22086962 wikiPageWikiLink Q5961.
- Q22086962 wikiPageWikiLink Q7009396.
- Q22086962 wikiPageWikiLink Q7239412.
- Q22086962 wikiPageWikiLink Q7824699.
- Q22086962 wikiPageWikiLink Q8691170.
- Q22086962 comment "UW Coronae Borealis, also known as MS1603.6+2600, is a low mass X-ray binary star system located in the constellation Corona Borealis. Astronomer Simon Morris and colleagues discovered the X-ray source in 1990 and were able to match it up with a faint star with an average visual magnitude of 19.4. The system is thought to be made up of a neutron star that has an accretion disk that draws material from its companion, a star less massive than the Sun. The disk is asymmetrical.".
- Q22086962 label "UW Coronae Borealis".