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Characterization of the Praesepe Star Cluster by Photometry and Proper Motions with 2MASS, PPMXL, and Pan-STARRS

P. F. Wang,W. P. Chen,C. C. Lin,A. K. Pandey,C. K. Huang,N. Panwar,C. H. Lee, M. F. Tsai,C. -H. Tang,B. Goldman,W. S. Burgett,K. C. Chambers,P. W. Draper,H. Flewelling,T. Grav,J. N. Heasley,K. W. Hodapp,M. E. Huber,R. Jedicke,N. Kaiser,R. -P. Kudritzki,G. A. Luppino,R. H. Lupton,E. A. Magnier,N. Metcalfe,D. G. Monet,J. S. Morgan,P. M. Onaka,P. A. Price,C. W. Stubbs,W. Sweeney,J. L. Tonry,R. J. Wainscoat,C. Waters

Astrophysical journal/˜The œAstrophysical journal（2014）

Cited 28|Views65
Key words
open clusters and associations: individual (Praesepe),stars: kinematics and dynamics,stars:luminosity function, mass function
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