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20152023
most citedCan we constrain interior structure of rocky exoplanets from mass and radius measurements?

353 citations · 2.9k across the 46 of their papers we have counts for

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Showing 2018Show all

9 papers · 1 filter

astro-ph.EP2018★ 97 cited

A new class of Super-Earths formed from high-temperature condensates: HD219134 b, 55 Cnc e, WASP-47 e

Caroline Dorn, John H. D. Harrison, Amy Bonsor +1

We hypothesise that differences in the temperatures at which the rocky material condensed out of the nebula gas can lead to differences in the composition of key rocky species (e.g…

astro-ph.EP2018★ 19 cited

Mass, radius, and composition of the transiting planet 55 Cnc e : using interferometry and correlations --- A quick update

Aurélien Crida, Roxanne Ligi, Caroline Dorn +2

In a recent paper (Crida et al. 2018, accepted on April 19), we presented a method to derive the mass and radius of a transiting exoplanet and their intrinsic correlation, that we…

astro-ph.EP2018★ 36 cited

Equation of state of SiC at extreme conditions: new insight into the interior of carbon rich exoplanets

F. Miozzi, G. Morard, D. Antonangeli +5

There is a direct relation between the composition of a host star and that of the planets orbiting around it. As such, the recent discovery of stars with unusual chemical compositi…

astro-ph.EP2018★ 57 cited

Interior characterization in multiplanetary systems: TRAPPIST-1

Caroline Dorn, Klaus Mosegaard, Simon L Grimm +1

Interior characterization traditionally relies on individual planetary properties, ignoring correlations between different planets of the same system. For multi-planetary systems,…

astro-ph.EP2018★ 129 cited

The 55 Cnc system reassessed

V. Bourrier, X. Dumusque, C. Dorn +9

Orbiting a bright, nearby star the 55 Cnc system offers a rare opportunity to study a multiplanet system that has a wide range of planetary masses and orbital distances. Using two…

astro-ph.EP2018★ 35 cited

Absolute densities in exoplanetary systems: photodynamical modelling of Kepler-138

J. M. Almenara, R. F. Díaz, C. Dorn +2

In favourable conditions, the density of transiting planets in multiple systems can be determined from photometry data alone. Dynamical information can be extracted from light curv…