Abstract
We estimate the thin-disk scale height of the Galactic population of L and T dwarfs based on star counts from 15 deep parallel fields from the Hubble Space Telescope. From these observations, we have identified 28 candidate L and T dwarfs based on their i′-z′ color and morphology. By comparing these star counts with a simple Galactic model, we estimate the scale height to be 350 ± 50 pc, which is consistent with the increase in vertical scale with decreasing stellar mass and is independent of reddening, color-magnitude limits, and other Galactic parameters. With this refined measure, we predict that less than 109 M⊙ of the Milky Way can be in the form of L and T dwarfs and confirm that high-latitude, z ≃6 galaxy surveys that use the i′-band dropout technique are 97%-100% free of L and T dwarf interlopers.
Original language | English (US) |
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Pages (from-to) | L159-L162 |
Journal | Astrophysical Journal |
Volume | 631 |
Issue number | 2 II |
DOIs | |
State | Published - Oct 1 2005 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science