The Lambda Orionis Star Forming Region: a Test for the Universality of the IMF

Details The Lambda Orionis Star Forming Region: a Test for the Universality of the IMF The Lambda Orionis Star Forming Region: a Test for the Universality of the IMF

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..195b&link_type=abstract

XMM-Newton Proposal ID #04052106

Physics

Stars, White Dwarfs, Solar System, Barnard30, Barnard30-South, Barnard35, Ldn1588, Ldn1603, Collinder69-Eas, Xmm-Newton Proposal 04052106

Scientific paper

We propose observations with XMM-EPIC/MOS in five distinct sibling associations belonging to the Lambda Orionis Star Forming Region (2--5 Myr, 340 pc). We have already optical, near-IR, and Spitzer photometry, and spectroscopy for objects down to 0.015 M(sun). The goals are: i) Assess the membership of our candidates and detect new members. ii) Derive accurate IMFs for each association, checking the universality of the IMF. iii) Study the properties and evolution of the X-ray Luminosity Functions.

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