Further evidence of a brown dwarf orbiting the post-common envelope eclipsing binary V470 cam (HS 0705+6700)
Several post-common envelope binaries have slightly increasing, decreasing or oscillating orbital periods. One of several possible explanations is light travel-time changes, caused by the binary centre-of-mass being perturbed by the gravitational pull of a third body. Further studies are necessary b...
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| Format: | Journal article |
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De Gruyter
2017
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