Peter Woitke
- Too little radiation pressure on dust in the winds of oxygen-rich AGB stars
2006/09/14 by P. Woitke, Peter Woitke · 10 citations
Physics and Astronomy · #Astro and Planetary Science #Astrophysics #Astrophysics and Star Formation Studies #Asymptotic giant branch #Circumstellar dust #Condensation #Nucleation #Opacity #Oxygen #Physics #Radiative transfer #Stars #Stellar, planetary, and galactic studies #Thermodynamics #astro-ph
- Radiation thermo-chemical models of protoplanetary disks I. Hydrostatic disk structure and inner rim
2009/04/02 by Peter Woitke, Inga Kamp, Wing-Fai Thi · 2 citations
Physics and Astronomy · #astro-ph.EP #astro-ph.SR
- Radiation thermo-chemical models of protoplanetary discs
2012/10/29 by Wing-Fai Thi, W.‐F. Thi, I. Kamp +9 · 2 citations
Chemistry · Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Carbon monoxide #Chemistry #Context (archaeology) #Geology #Materials science #Molecular Spectroscopy and Structure #Optics #Photochemistry #Physics #Radiation #Stars #T Tauri star #Ultraviolet #astro-ph.GA
- Consistent dust and gas models for protoplanetary disks: II. Chemical networks and rates
2017/07/23 by Inga Kamp, Wing-Fai Thi, Peter Woitke +3 · 2 citations
Physics and Astronomy · #astro-ph.SR #astro-ph.GA
- 2D models for dust-driven AGB star winds
2006/02/16 by P. Woitke, Peter Woitke · 2 citations
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Circumstellar dust #Cosmic dust #Hydrostatic equilibrium #Physics #Radiation pressure #Radiative transfer #Solar and Space Plasma Dynamics #Stars #Stellar, planetary, and galactic studies #astro-ph
- The protoplanetary disk of FT Tauri: multiwavelength data analysis and modeling
2014/05/29 by Antonio Garufi, A. Garufi, Linda Podio +17 · 1 citation
Chemistry · Physics and Astronomy · #Astrophysics and Star Formation Studies #Molecular Spectroscopy and Structure #Stellar, planetary, and galactic studies #astro-ph.EP #astro-ph.SR