activity
19952022
most citedA Non-Gray Theory of Extrasolar Giant Planets and Brown Dwarfs

1.4k citations · 13.1k across the 92 of their papers we have counts for

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Showing 2012Show all

7 papers · 1 filter

astro-ph.SR2012★ 83 cited

A Comparison of Near-Infrared Photometry and Spectra for Y Dwarfs with a New Generation of Cool Cloudy Models

S. K. Leggett, Caroline V. Morley, M. S. Marley +3

We present YJHK photometry, or a subset, for the six Y dwarfs discovered in WISE data by Cushing et al.. The data were obtained using NIRI on the Gemini North telescope. We also pr…

astro-ph.SR2012

Towards an Understanding of the Atmospheres of Cool White Dwarfs

Piotr M. Kowalski, Didier Saumon, Jay Holberg +1

Cool white dwarfs with Teff < 6000 K are the remnants of the oldest stars that existed in our Galaxy. Their atmospheres, when properly characterized, can provide valuable informati…

astro-ph.SR2012★ 453 cited

Neglected Clouds in T and Y Dwarf Atmospheres

Caroline V. Morley, Jonathan J. Fortney, Mark S. Marley +3

As brown dwarfs cool, a variety of species condense in their atmospheres, forming clouds. Iron and silicate clouds shape the emergent spectra of L dwarfs, but these clouds dissipat…

astro-ph.EP2012★ 285 cited

Masses, Radii, and Cloud Properties of the HR 8799 Planets

Mark S. Marley, Didier Saumon, Michael Cushing +3

The near-infrared colors of the planets directly imaged around the A star HR 8799 are much redder than most field brown dwarfs of the same effective temperature. Previous theoretic…

astro-ph.SR2012★ 138 cited

New H2 collision-induced absorption and NH3 opacity and the spectra of the coolest brown dwarfs

D. Saumon, M. S. Marley, M. Abel +2

We present new cloudy and cloudless model atmospheres for brown dwarfs using recent ab initio calculations of the line list of ammonia (NH3) and of the collision-induced absorption…

astro-ph.SR2012★ 73 cited

The Properties of the 500 K Dwarf UGPS J072227.51-054031.2, and a Study of the Far-Red Flux of Cold Brown Dwarfs

S. K. Leggett, D. Saumon, M. S. Marley +15

We present i and z photometry for 25 T dwarfs and one L dwarf. Combined with published photometry, the data show that the i - z, z - Y and z - J colors of T dwarfs are very red, an…