activity
20102023
most citedKepler planets: a tale of evaporation

802 citations · 7.6k across the 87 of their papers we have counts for

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Showing 2020Show all

11 papers · 1 filter

astro-ph.EP2020★ 71 cited

Hydrogen dominated atmospheres on terrestrial mass planets: evidence, origin and evolution

J. E. Owen, I. F. Shaikhislamov, H. Lammer +2

The discovery of thousands of highly irradiated, low-mass, exoplanets has led to the idea that atmospheric escape is an important process that can drive their evolution. Of particu…

astro-ph.EP2020★ 148 cited

The nature and origins of sub-Neptune size planets

Jacob L. Bean, Sean N. Raymond, James E. Owen

Planets intermediate in size between the Earth and Neptune, and orbiting closer to their host stars than Mercury does the Sun, are the most common type of planet revealed by exopla…

astro-ph.EP2020★ 46 cited

Constraining the entropy of formation from young transiting planets

James E. Owen

Recently K2 and TESS have discovered transiting planets with radii between 5-10 R around stars with ages Myr. These young planets are likely to be the progen…

astro-ph.EP2020★ 87 cited

A review of possible planetary atmospheres in the TRAPPIST-1 system

Martin Turbet, Emeline Bolmont, Vincent Bourrier +4

TRAPPIST-1 is a fantastic nearby (~39.14 light years) planetary system made of at least seven transiting terrestrial-size, terrestrial-mass planets all receiving a moderate amount…

astro-ph.EP2020★ 9 cited

Unveiling the Planet Population at Birth

James G. Rogers, James E. Owen

The radius distribution of small, close-in exoplanets has recently been shown to be bimodal. The photoevaporation model predicted this bimodality. In the photoevaporation scenario,…

astro-ph.EP2020★ 39 cited

Snow-lines can be thermally unstable

James E. Owen

Volatile species in protoplanetary discs can undergo a phase change from vapour to solid. These "snow-lines" can play vital roles in planet formation at all scales, from dust coagu…