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19972005
most citedYoung, Jupiter-Mass Objects in Ophiuchus

1 citations · 1 across the 3 of their papers we have counts for

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astro-ph20051 cited

Young, Jupiter-Mass Objects in Ophiuchus

K. N. Allers, D. T. Jaffe, N. S. van der Bliek +2

We have used 3.5 to 8 micron data from the Cores to Disks (c2d) Legacy survey and our own deep IJHKs images of a 0.5 square degree portion of the c2d fields in Ophiuchus to produce…

astro-ph2005

Pulsations induced by deuterium-burning in young brown dwarfs

Francesco Palla, Isabelle Baraffe

Very low-mass stars and brown dwarfs can undergo pulsational instability excited by central deuterium burning during the initial phases of their evolution. We present the results o…

astro-ph2004

The physics of extrasolar gaseous planets : from theory to observable signatures

G. Chabrier, F. Allard, I. Baraffe +2

We review our present understanding of the physical properties of substellar objects, brown dwarfs and irradiated or non-irradiated gaseous exoplanets. This includes a description…

astro-ph2000

Pre-Main Sequence models for low-mass stars and brown dwarfs

I. Baraffe, G. Chabrier, F. Allard +1

We present evolutionary models for low mass stars and brown dwarfs ($m \le 1.2 \msol$) based on recent improvement of the theory: equation of state, atmosphere models, ... We conce…

astro-ph1998

Discovery of a Very Low-Mass Binary with HST/NICMOS

E. L. Martin, G. Basri, W. Brandner +7

Hubble Space Telescope NICMOS observations are presented of six brown dwarf candidates in the Pleiades open cluster. One of them, namely CFHT-Pl-18, is clearly resolved as a binary…

astro-ph1998

The CV Period Minimum

Ulrich Kolb, Isabelle Baraffe

Using improved, up-to-date stellar input physics tested against observations of low-mass stars and brown dwarfs we calculate the secular evolution of low-mass donor CVs, including…