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20012026
most citedThe imprint of exoplanet formation history on observable present-day spectra of hot Jupiters

391 citations · 4.6k across the 83 of their papers we have counts for

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Showing 2015Show all

5 papers · 1 filter

astro-ph.SR2015★ 15 cited

A multi-wavelength interferometric study of the massive young stellar object IRAS 13481-6124

Paul A. Boley, Stefan Kraus, Willem-Jan de Wit +7

We present new mid-infrared interferometric observations of the massive young stellar object IRAS 13481-6124, using VLTI/MIDI for spectrally-resolved, long-baseline measurements (p…

astro-ph.SR2015★ 138 cited

A Keplerian-like disk around the forming O-type star AFGL 4176

Katharine G. Johnston, Thomas P. Robitaille, Henrik Beuther +6

We present Atacama Large Millimeter/submillimeter Array (ALMA) line and continuum observations at 1.2mm with ~0.3" resolution that uncover a Keplerian-like disk around the forming…

astro-ph.EP2015★ 235 cited

Model atmospheres of irradiated exoplanets: The influence of stellar parameters, metallicity, and the C/O ratio

Paul Mollière, Roy van Boekel, Cornelis Petrus Dullemond +2

Many parameters constraining the spectral appearance of exoplanets are still poorly understood. We therefore study the properties of irradiated exoplanet atmospheres over a wide pa…

astro-ph.EP2015★ 94 cited

Scattered light images of spiral arms in marginally gravitationally unstable discs with an embedded planet

A. Pohl, P. Pinilla, M. Benisty +5

Scattered light images of transition discs in the near-infrared often show non-axisymmetric structures in the form of wide-open spiral arms in addition to their characteristic low-…

astro-ph.SR2015★ 97 cited

The structure of disks around intermediate-mass young stars from mid-infrared interferometry. Evidence for a population of group II disks with gaps

J. Menu, R. van Boekel, Th. Henning +3

The disks around Herbig Ae/Be stars are commonly divided into group I and group II based on their far-infrared spectral energy distribution, and the common interpretation for that…