Abstract
The observational characterization of the stellar mass function in galactic clusters, the field, and even other galaxies, has resulted in a wealth of parameters that must be reproduced and explained by any successful star formation theory. To extend our knowledge on the mass function to the substellar regime, we have conducted a large observational survey of nearby young clusters (ρ Oph, IC 348, Serpens, and λ Ori). We adopted a twofold approach to this study, using both near-IR photometry to find all candidate substellar members and extensive spectroscopic follow-up to derive a spectroscopic IMF, and deep methane imaging to search for the lowest mass members. I will present the results of this longterm endeavor, where we have found no evidence for variations in the substellar mass function across different clusters, and have uncovered a handful of candidate young T dwarfs likely to represent the minimum mass for star formation.
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Alves de Oliveira, C. Alves de Oliveira, C., Moraux, E., Bouvier, J., et al. 2010, A&A, 515, A75
Alves de Oliveira C., Moraux E., Bouvier J., Bouy H., 2012, A&A, 539, A151
Burgess, A. S. M., Moraux, E., Bouvier, J., Marmo, C., Albert, L., & Bouy, H. 2009, A&A, 508, 823
Spezzi, L., Alves de Oliveira, C., Moraux, E., Bouvier, J., Winston, E., Hudelot, P., Bouy, H., Cuillandre, J.-C., 2012, A&A, in press
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de Oliveira, C.A. et al. (2014). The Low Mass End of the IMF Unveiled by the WIRCam/CFHT Survey of Nearby Young Clusters. In: Stamatellos, D., Goodwin, S., Ward-Thompson, D. (eds) The Labyrinth of Star Formation. Astrophysics and Space Science Proceedings, vol 36. Springer, Cham. https://doi.org/10.1007/978-3-319-03041-8_68
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DOI: https://doi.org/10.1007/978-3-319-03041-8_68
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