Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-03-14
Astronomy and Astrophysics
Astrophysics
ApJL, in press
Scientific paper
10.1086/320017
We use three field L and T dwarfs which were discovered to be wide companions to known stars by the Two Micron All-Sky Survey (2MASS) to derive a preliminary brown dwarf companion frequency. Observed L and T dwarfs indicate that brown dwarfs are not unusually rare as wide (Delta >1000 A.U.) systems to F-M0 main-sequence stars (M>0.5M_sun, M_V<9.5), even though they are rare at close separation (Delta <3 A.U.), the ``brown dwarf desert.'' Stellar companions in these separation ranges are equally frequent, but brown dwarfs are >~ 10 times as frequent for wide than close separations. A brown dwarf wide-companion frequency as low as the 0.5% seen in the brown dwarf desert is ruled out by currently-available observations.
Burgasser Adam
Gizis John E.
Kirkpatrick Joseph D.
Liebert James
Monet David G.
No associations
LandOfFree
Substellar Companions to Main Sequence Stars: No Brown Dwarf Desert at Wide Separations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Substellar Companions to Main Sequence Stars: No Brown Dwarf Desert at Wide Separations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Substellar Companions to Main Sequence Stars: No Brown Dwarf Desert at Wide Separations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-176030