A RAVE investigation on Galactic open clusters I. Radial velocities and metallicities
Context. Galactic open clusters (OCs) mainly belong to the young stellar population in the Milky Way disk, but are there groups and complexes of OCs that possibly define an additional level in hierarchical star formation? Current compilations are too incomplete to address this question, especially regarding radial velocities (RVs) and metallicities ([M/H]). Aims. Here we provide and discuss newly obtained RV and [M/H] data, which will enable us to reinvestigate potential groupings of open...[Show more]
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
|01_Conrad_A_RAVE_investigation_on_2014.pdf||3.94 MB||Adobe PDF||Request a copy|
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