activity
19982024
most citedDUst Around NEarby Stars. The survey observational results

220 citations · 1.6k across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.GA2024

Trapped Water on Silicates in the Laboratory and in Astrophysical Environments

Alexey Potapov, Cornelia Jäger, Harald Mutschke +1

Existence of strongly bound water molecules on silicate surfaces, above the desorption temperature of water ice, has been first predicted by computational studies and recently demo…

astro-ph.EP2022★ 10 cited

Sub-mm/mm optical properties of real protoplanetary matter derived from Rosetta/MIRO observations of comet 67P

Johanna Bürger, Thilo Glißmann, Anthony Lethuillier +6

Optical properties are required for the correct understanding and modelling of protoplanetary and debris discs. By assuming that comets are the most pristine bodies in the solar sy…

astro-ph.EP2019★ 18 cited

Constraining the detectability of water ice in debris disks

Minjae Kim, Sebastian Wolf, Alexey Potapov +2

Water ice is important for the evolution and preservation of life. Identifying the distribution of water ice in debris disks is therefore of great interest in the field of astrobio…

astro-ph.GA2019★ 43 cited

Dust absorption and scattering in the silicon K-edge

S. T. Zeegers, E. Costantini, D. Rogantini +5

The composition and properties of interstellar silicate dust are not well understood. In X-rays, interstellar dust can be studied in detail by making use of the fine structure feat…

astro-ph.GA2018★ 21 cited

Low temperature optical properties of interstellar and circumstellar icy silicate grain analogues in the mid-infrared spectral region

Alexey Potapov, Harald Mutschke, Phillip Seeber +2

Two different silicate/water ice mixtures representing laboratory analogues of interstellar and circumstellar icy grains were produced in the laboratory. For the first time, optica…

astro-ph.HE2017★ 40 cited

Investigating the interstellar dust through the Fe K-edge

D. Rogantini, E. Costantini, S. T. Zeegers +5

The chemical and physical properties of interstellar dust in the densest regions of the Galaxy are still not well understood. X-rays provide a powerful probe since they can penetra…