Radial velocity monitoring of PG 1018-047
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https://b2find.eudat.eu/dataset/9fbaf0e7-245e-5456-a21b-a3d3065721cf
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About 50 per cent of all known hot subdwarf B stars (sdBs) reside in close (short-period) binaries, for which common-envelope ejection is the most likely formation mechanism....
