Lambda Orionis: A 0.02-50 Msun Initial Mass Function

Details Lambda Orionis: A 0.02-50 Msun Initial Mass Function Lambda Orionis: A 0.02-50 Msun Initial Mass Function

2004-09-21

arxiv.org/abs/astro-ph/0409499v1

Astronomy and Astrophysics

Astrophysics

Contributed talk presented at the conference on "IMF@50: The Stellar Initial Mass Function Fifty Years Later" held at Abbazia

Scientific paper

The Lambda Orionis Star Forming Region is dominated by the O8 III star lambda^1 Ori. Among other structures, it includes a CO and a dust ring whose diameter is about nine deg, the S264 HII region, a large number of IRAS sources, the Barnard 30 and 35 dark clouds and a cluster associated with the central star, the Lambda Ori cluster (Collinder 69). We derive the initial mass function for this cluster (~5 Myr), covering several orders of magnitude in mass (50 - 0.02 Msun).

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