We present results of a search for nearby star clusters and associatio
ns using Hipparcos Catalogue data, restricting the sample to stars wit
h parallaxes above 2 mas (d less than or similar to 500 pc). Two new O
B associations have been identified in the Carina-Vela and Cepheus-Cyg
nus-Lyra-Vulpecula regions. A very probable new open cluster has been
discovered in Carina. The cluster, a Car, named after its brightest me
mber, is young (60 Myr) and nearby (d = 132 pc). However, only seven b
ona fide members can be drawn from the Hipparcos data. We report a det
ection of nine open cluster candidates in the distance range of 150 to
400 pc, and six possible associations almost all located within the G
ould belt, although slightly older than the known nearby associations.
In all cases, we present Yale theoretical isochrone fits to the color
-magnitude diagrams, which indicate a moderate spread of ages between
60 to 200 Myr. Evidently, these young open cluster and association can
didates are related to the overall distribution of young OB and A-type
stars in the solar neighborhood.