activity
19952023
most citedA Non-Gray Theory of Extrasolar Giant Planets and Brown Dwarfs

1.4k citations · 36k across the 266 of their papers we have counts for

collaborators
Showing 2011Show all

11 papers · 1 filter

astro-ph.EP2011★ 133 cited

Analytic models for albedos, phase curves and polarization of reflected light from exoplanets

Nikku Madhusudhan, Adam Burrows

New observational facilities are becoming increasingly capable of observing reflected light from transiting and directly imaged extrasolar planets. In this study, we provide an ana…

astro-ph.SR2011★ 87 cited

The Hydrodynamic Origin of Neutron Star Kicks

J. Nordhaus, T. Brandt, A. Burrows +1

We present results from a suite of axisymmetric, core-collapse supernova simulations in which hydrodynamic recoil from an asymmetric explosion produces large proto-neutron star (PN…

astro-ph.EP2011★ 80 cited

Warm Spitzer Photometry of XO-4b, HAT-P-6b and HAT-P-8b

Kamen O. Todorov, Drake Deming, Heather A. Knutson +11

We have analyzed Warm Spitzer/IRAC observations of the secondary eclipses of three planets, XO-4b, HAT-P-6b and HAT-P-8b. We measure secondary eclipse amplitudes at 3.6μm and 4.5μm…

astro-ph.EP2011★ 15 cited

Day and night side core cooling of a strongly irradiated giant planet

J. Budaj, I. Hubeny, A. Burrows

The internal heat loss, or cooling, of a planet determines its structure and evolution. We study the effects of irradiation, metallicity of the atmosphere, heat redistribution, str…

astro-ph.EP2011★ 52 cited

The Impact of Circumplantary Jets on Transit Spectra and Timing Offsets for Hot-Jupiters

Ian Dobbs-Dixon, Eric Agol, Adam Burrows

We present theoretical wavelength-dependent transit light curves for the giant planet HD209458b based on a number of state of the art 3D radiative hydrodynamical models. By varying…

astro-ph.EP2011★ 374 cited

Spectral and Photometric Diagnostics of Giant Planet Formation Scenarios

David S. Spiegel, Adam Burrows

Gas-giant planets that form via core accretion might have very different characteristics from those that form via disk-instability. Disk-instability objects are typically thought t…