Matches in DBpedia 2015-10 for { ?s ?p "Ap and Bp stars are peculiar stars (hence the "p") of types A and B which show overabundances of some metals, such as strontium, chromium and europium; in addition, larger overabundances are often seen in praseodymium and neodymium. These stars have a much slower rotation than normal for A and B-type stars, although some exhibit rotation velocities up to about 100 kilometers per second."@en }
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- Ap_and_Bp_stars abstract "Ap and Bp stars are peculiar stars (hence the "p") of types A and B which show overabundances of some metals, such as strontium, chromium and europium; in addition, larger overabundances are often seen in praseodymium and neodymium. These stars have a much slower rotation than normal for A and B-type stars, although some exhibit rotation velocities up to about 100 kilometers per second.".
- Ap_and_Bp_stars comment "Ap and Bp stars are peculiar stars (hence the "p") of types A and B which show overabundances of some metals, such as strontium, chromium and europium; in addition, larger overabundances are often seen in praseodymium and neodymium. These stars have a much slower rotation than normal for A and B-type stars, although some exhibit rotation velocities up to about 100 kilometers per second.".