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D.J. James, K.G Keivan (Vanderbilt University), R.D. Jeffries (Keele University), N.H. Hambly (Royal Observatory Edinburgh), J-C Mermilliod (Observatoire de Genève), S Meibom (University of Wisconsin-Madison), C Deliyannis (Indiana University)
We present the results of a large-scale photometric and kinematic survey of the intermediate age (220 Myr) open cluster NGC 6475 (M7). We present optical and infra-red photomtetry over 1 sq. degree with complimentary multi-epoch radial velocities for some 750-odd photometric members to define a sample of probable single, probable binary and possible single members and non-members. Cluster properties of the single and binary members are discussed.
The author(s) of this abstract have provided an email address for comments about the abstract: djj@estrella.phy.vanderbilt.edu
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Bulletin of the American Astronomical Society, 36 #2
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