Establishing Solar-type Membership Of The Young (100 Myr) Open Cluster Blanco 1

Details Establishing Solar-type Membership Of The Young (100 Myr) Open Cluster Blanco 1 Establishing Solar-type Membership Of The Young (100 Myr) Open Cluster Blanco 1

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.1609j&link_type=abstract

American Astronomical Society Meeting 210, #16.09; Bulletin of the American Astronomical Society, Vol. 39, p.117

Astronomy and Astrophysics

Astronomy

Scientific paper

New wide-field UBVI photometric observations are used in concert with astrometric (proper motions) and kinematic studies (radial velocities) to establish the solar-type star membership of the interesting Galactic open cluster Blanco 1 (Zeta Sculptoris).
Membership criteria are applied to distinguish between single and binary stars to allow us to correctly interpret a follow-up study of lithium abundance and X-ray activity.
These Blanco 1 datasets are to be used in comparison to the well studied Alpha Persei, Pleiades and NGC 2516 clusters in order to study early-main sequence stellar evolution.

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