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J/A+A/409/147 J magnitude of IC 348 brown dwarfs (Preibisch+, 2003)
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Constraints on the IMF and the brown dwarf population of the young
cluster IC 348.
Preibisch T., Stanke T., Zinnecker H.
<Astron. Astrophys. 409, 147 (2003)>
=2003A&A...409..147P
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ADC_Keywords: Clusters, open ; Stars, pre-main sequence ; Photometry
Keywords: stars: pre-main sequence - stars: low-mass, brown dwarfs -
stars: luminosity function, mass function -
open clusters and associations: general
Abstract:
We use a deep near-infrared census of the young stellar cluster IC 348
to construct and analyze its luminosity function. Our mosaic image of
IC 348 covers the full extent of the cluster with a completeness limit
of J 19.5 and is therefore sensitive for 2Myr old cluster members with
masses as low as M>=0.005M_sun_ or the mean extinction of the known
cluster members (A_V_ 3.5mag).
Description:
The observations discussed in this paper were obtained during the
night of 2nd Dec. 2001 using the Omega Prime wide-field near-infrared
camera on the Calar Alto 3.5m telescope in service observing mode.