Zobrazeno 1 - 6
of 6
pro vyhledávání: '"S. M. Stammler"'
Autor:
P. Pinilla, Th. Henning, E. Miller, T. Birnstiel, S. M. Stammler, Sebastian Marino, Christian T. Lenz
The question of what determines the width of Kuiper belt analogues (exoKuiper belts) is an open one. If solved, this understanding would provide valuable insights into the architecture, dynamics, and formation of exoplanetary systems. Recent observat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b17431070750b10f154ed0d49387113
http://arxiv.org/abs/2110.04007
http://arxiv.org/abs/2110.04007
Publikováno v:
Astronomy & Astrophysics
Pebble accretion is an emerging paradigm for the fast growth of planetary cores. Pebble flux and pebble sizes are the key parameters used in the pebble accretion models. We aim to derive the pebble sizes and fluxes from state-of-the-art dust coagulat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5046260230aad9e1380fe8cc23e057aa
Publikováno v:
Astronomy & Astrophysics. 640:A61
Context. When we wish to understand planetesimal formation, the only data set we have is our own Solar System. The Solar System is particularly interesting because so far, it is the only planetary system we know of that developed life. Understanding
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e0f303bcb19004e1fd6b720d3b1e9722
https://doi.org/10.1051/0004-6361/202037878
https://doi.org/10.1051/0004-6361/202037878
Autor:
Hubert Klahr, Cornelis P. Dullemond, Til Birnstiel, Sean M. Andrews, Joanna Drazkowska, S. M. Stammler
Publikováno v:
The Astrophysical Journal
Recent high-resolution interferometric observations of protoplanetary disks at (sub-)millimeter wavelengths reveal omnipresent substructures, such as rings, spirals, and asymmetries. A detailed investigation of eight rings detected in five disks by t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::46f5ab98783a2248a05083b4cd1c004b
Context. Despite the recent discovery of spiral-shaped features in protoplanetary discs in the near-infrared and millimetric wavelengths, there is still an active discussion to understand how they formed. In fact, the spiral waves observed in discs a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ec0804214e9f2154707b433eb4a2d1ac
http://arxiv.org/abs/1811.08441
http://arxiv.org/abs/1811.08441
Publikováno v:
Astrophysical Journal; 8/10/2017, Vol. 845 Issue 1, p1-1, 1p