Accession Number : ADA622437


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


Descriptive Note : Journal article


Corporate Author : NAVAL OBSERVATORY FLAGSTAFF AZ


Personal Author(s) : Wang, P F ; Chen, W P ; Lin, C C ; Pandey, A K ; Huang, C K ; Panwar, N ; Lee, C H ; Tsai, M F ; Tang, C -H ; Goldman, B


Full Text : https://apps.dtic.mil/dtic/tr/fulltext/u2/a622437.pdf


Report Date : 20 Mar 2014


Pagination or Media Count : 11


Abstract : Membership identification is the first step in determining the properties of a star cluster. Low-mass members in particular could be used to trace the dynamical history, such as mass segregation, stellar evaporation, or tidal stripping, of a star cluster in its Galactic environment. We identified member candidates of the intermediate-age Praesepe cluster (M44) with stellar masses 0.11-2.4 solar masses, using Panoramic Survey Telescope And Rapid Response System and Two Micron All Sky Survey photometry, and PPMXL proper motions. Within a sky area of 3 deg radius, 1040 candidates are identified, of which 96 are new inclusions. Using the same set of selection criteria on field stars, an estimated false positive rate of 16% was determined, suggesting that 872 of the candidates are true members. This most complete and reliable membership list allows us to favor the BT-Settl model over other stellar models. The cluster shows a distinct binary track above the main sequence, with a binary frequency of 20%-40%, and a high occurrence rate of similar mass pairs. The mass function is consistent with that of the disk population but shows a deficit of members below 0.3 solar masses. A clear mass segregation is evidenced, with the lowest-mass members in our sample being evaporated from this disintegrating cluster.


Descriptors :   *STARS , DYNAMICS , IDENTIFICATION , PHOTOMETRY


Subject Categories : Astrophysics


Distribution Statement : APPROVED FOR PUBLIC RELEASE