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Self-consistent ice opacities in disk modelsarXiv
arxiv.org
von AM Arabhavi · · Zitiert von: 2 — Ices in planet-forming disks: Self-consistent ice opacities in disk models. Authors:Aditya M. Arabhavi, Peter Woitke, Stephanie M. Cazaux, Inga ...
Dust-driven Winds Beyond Spherical SymmetryHarvard University
adsabs.harvard.edu
von P Woitke · · Zitiert von: 2 — ... toward RGB Peter Woitke stars and K giants without a clear cut-off, which would be expected if all these winds were actually dust-driven.
Homogenitätsanalyse von Metallspuren in ...Wiley
onlinelibrary.wiley.com
von G Henrion · · Zitiert von: 5 — Peter Woitke,. Peter Woitke. Humboldt-Universität zu Berlin, Sektion Chemie, Berlin, -2. Search for more papers by this author.
Use of a Mercury Bubble Electrode for preparative organic electrolysisonlinelibrary.wiley.com › abs › prac
onlinelibrary.wiley.com
von F Pragst · · Zitiert von: 2 — Peter Woitke,. Peter Woitke. Humboldt-Universität zu Berlin, Sektion Chemie, DDR Berlin, –2. Search for more papers by this author.
Erratum: "Consistent Simulations of Substellar Atmospheres ...Institute of Physics
iopscience.iop.org
von C Helling · · Zitiert von: 13 — Christiane Helling, Matthias Dehn, Peter Woitke, and Peter H. Hauschildt. © The American Astronomical Society. All rights reserved. Printed in U.S.A.
arXiv:astro-ph v1 14 Sep 2006CORE
core.ac.uk
von P Woitke · · Zitiert von: 255 — Peter Woitke: Too little radiation pressure on dust in winds of oxygen-rich AGB stars. Fig. 1. Extinction efficiencies over particle radius ...
Dynamics and Instabilities in Dusty Winds | SpringerLinkspringer.com
link.springer.com
von Y Simis · · Zitiert von: 2 — Yvonne Simis &; Peter Woitke. Chapter Accesses. 4 Citations. Part of the Astronomy and Astrophysics Library book series (AAL) ...
The Chaotic Winds of AGB Stars: Observation Meets Theorylink.springer.com › chapter
link.springer.com
von P Woitke · · Zitiert von: 1 — Peter Woitke &; Andreas Quirrenbach. Conference paper Accesses. 1 Citations. Part of the Eso Astrophysics Symposia book series (ESO) ...
Atmospheres of Rocky Exoplanets Stability of liquid water ...ku.dk
cels.nbi.ku.dk
von O Herbort · Zitiert von: 23 — Atmospheres of Rocky Exoplanets. Stability of liquid water and cloud predictions. Oliver Herbort. Supervisor: Peter Woitke, Aubrey Zerkle.
Dust formation in brown dwarf atmospheres under ...KOBV
opus4.kobv.de
von C Helling · · Zitiert von: 1 — Christiane Helling, Rupert Klein, Peter Woitke, Erwin Sedlmayr. Based on the knowledge gained from direct numerical simulations which are only possible in ...
Heating and cooling processes in disksProQuest
search.proquest.com
von P Woitke · · Zitiert von: 13 — The resulting thermal structure of protoplanetary disks is described and discussed. Full Text. Heating and cooling processes in disks Peter Woitke 1SUPA, School ...
Disk Evolution, Element Abundances and Cloud Properties MDPIwww.mdpi.com › ...
www.mdpi.com
von C Helling · · Zitiert von: 89 — Disk Evolution, Element Abundances and Cloud Properties of Young Gas Giant Planets. by. Christiane Helling. 1,*,. Peter Woitke. 1,.
Modelling the Mass Loss of Cool AGB Stars | Symposiumwww.cambridge.org › core › journals › article › mo...
www.cambridge.org
von P Woitke · · Zitiert von: 21 — Modelling the Mass Loss of Cool AGB Stars. Published online by Cambridge University Press: 26 May Peter Woitke. Show author details ...
Self-consistent ice opacities in disk modelstudelft.nl
research.tudelft.nl
von AM Arabhavi · · Zitiert von: 2 — ... in planet-forming disks: Self-consistent ice opacities in disk models. A. M. Arabhavi, Peter Woitke, S.M. Cazaux, Inga Kamp, Christian Rab, Wing-Fai Thi.
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