Abstract
A large area deep survey for brown dwarfs from digitally stacked 1.2m Schmidt plates has revealed a population of very red stars (R-I>3). On the basis of their colours, near IR spectra and their luminosity estimates from proper motions, these objects appeared to be Brown Dwarfs. First measurements of the parallaxes of 8 of the reddest objects at the 1.5 danish telescope confirmed this, and showed that four of them have K-band luminosities some mags below the bottom of the main sequence. We present here those results.
| Original language | English |
|---|---|
| Title of host publication | In: Brown Dwarfs and Extrasolar Planets - ASP Conf Series 134 |
| Publisher | Astronomical Society of the Pacific |
| Pages | 106-8 |
| ISBN (Print) | 1-886733-54-6 |
| Publication status | Published - 1998 |
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