Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-08-25
Astrophys.J.631:L159-L162,2005
Astronomy and Astrophysics
Astrophysics
4 pages, 4 figures, accepted to ApJL
Scientific paper
10.1086/497368
We estimate the thin disk scale height of the Galactic population of L- & 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- & T- dwarfs based on their (i'-z') color and morphology. By comparing these star counts to a simple Galactic model, we estimate the scale height to be 350+-50 pc that 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 10^9 M_{sol} of the Milky Way can be in the form L- & T- dwarfs, and confirm that high-latitude, z~6 galaxy surveys which use the i'-band dropout technique are 97-100% free of L- & T- dwarf interlopers.
Cohen Seth H.
Hathi Nimish P.
Ryan Russell E. Jr.
Windhorst Rogier A.
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