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- W33594069 abstract "Recent studies of the substellar population in the Taurus cloud have revealed a deficit of substellar objects by a factor ' 2 compared to the Trapezium cluster population (Briceno et al. 1998; Luhman 2000). If confirmed, the higher low-mass cutoff in Taurus could have strong implications on IMF and substellar formation models. However, all studies to date have concentrated on the highest stellar density regions of the Taurus cloud. Reipurth & Clarke (2001) have proposed that brown dwarfs are stellar embryos ejected from their birth site early in their evolution. In order to test this scenario and investigate a possible spatial segregation between stars and brown dwarfs, we have performed a large scale optical survey of the Taurus cloud covering a total area of ' 30 deg2 down to a mass detection limits of 15 MJup. We first present results from a spectroscopic follow-up of a subsample of substellar candidates that revealed 4 new Brown Dwarfs and one Very Low Mass Taurus member. We then discuss the selection of candidates from a larger scale optical survey and the implications for the substellar IMF in Taurus." @default.
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- W33594069 date "2005-01-01" @default.
- W33594069 modified "2023-09-27" @default.
- W33594069 title "Exploring the substellar IMF in the Taurus cloud. New brown dwarfs in the Taurus star forming region" @default.
- W33594069 hasPublicationYear "2005" @default.
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