activity
20162019
most citedOvercoming the limitations of the energy-limited approximation for planet atmospheric escape

127 citations · 367 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2019★ 45 cited

Close-in sub-Neptunes reveal the past rotation history of their host stars: atmospheric evolution of planets in the HD3167 and K2-32 planetary systems

Daria Kubyshkina, Patricio Cubillos, Luca Fossati +7

Planet atmospheric escape induced by high-energy stellar irradiation is a key phenomenon shaping the structure and evolution of planetary atmospheres. Therefore, the present-day pr…

astro-ph.EP2019★ 21 cited

Transit Ly- signatures of terrestrial planets in the habitable zones of M dwarfs

K. G. Kislyakova, M. Holmström, P. Odert +6

We modeled the transit signatures in the Lya line of a putative Earth-sized planet orbiting in the HZ of the M dwarf GJ436. We estimated the transit depth in the Lya line for an ex…

astro-ph.EP2018★ 127 cited

Overcoming the limitations of the energy-limited approximation for planet atmospheric escape

Daria Kubyshkina, Luca Fossati, Nikolay V. Erkaev +6

Studies of planetary atmospheric composition, variability, and evolution require appropriate theoretical and numerical tools to estimate key atmospheric parameters, among which the…

astro-ph.EP2017★ 37 cited

Effect of stellar wind induced magnetic fields on planetary obstacles of non-magnetized hot Jupiters

N. V. Erkaev, P. Odert, H. Lammer +7

We investigate the interaction between the magnetized stellar wind plasma and the partially ionized hydrodynamic hydrogen outflow from the escaping upper atmosphere of non- or weak…

astro-ph.EP2017★ 65 cited

Escape and fractionation of volatiles and noble gases from Mars-sized planetary embryos and growing protoplanets

P. Odert, H. Lammer, N. V. Erkaev +6

Planetary embryos form protoplanets via mutual collisions, which can lead to the development of magma oceans. During their solidification, large amounts of the mantles' volatile co…

astro-ph.SR2016★ 72 cited

Identifying the "true" radius of the hot sub-Neptune CoRoT-24b by mass loss modelling

H. Lammer, N. V. Erkaev, L. Fossati +8

For the hot exoplanets CoRoT-24b and CoRoT-24c, observations have provided transit radii R of 3.70.4 R and 4.90.5 R, and masses of 5.…