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• W1998712918 abstract "UBVRI and Hα CCD photometry has been performed in the southern region of NGC 2264 around the Cone Nebula. A nearly complete list of pre–main-sequence (PMS) members in the cluster has been made from the compilation of Hα emission stars identified in this study plus those selected in previous investigations, together with stars with X-ray emission. Using the H-R diagram, we tested a set of four PMS evolution models based on the PMS age and age spread estimate for the cluster and the mass-age relationship among individual stars. The resultant initial mass function (IMF) is in good agreement with the field star IMF of the solar neighborhood, with an IMF slope Γ = -1.7 in the mass range 0.3 ≤ log m ≤ 0.8." @default.
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• W1998712918 date "2000-08-01" @default.
• W1998712918 modified "2023-09-23" @default.
• W1998712918 title "The Pre–Main-Sequence Stars and Initial Mass Function of NGC 2264" @default.
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• W1998712918 doi "https://doi.org/10.1086/301459" @default.
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