- Macroclumping as solution of the discrepancy between Hαand P v mass loss diagnostics for O-type stars
2013/10/01 by B. Šurlan, W. -R. Hamann, W.-R. Hamann +4 · 1 citation
Physics and Astronomy · Social Sciences · #Astronomical spectroscopy #Astronomy and Astrophysical Research #Educational Leadership and Practices #Hertzsprung–Russell diagram #O-type star #Resonance (particle physics) #Spectral line #Stars #Stellar atmosphere #Stellar wind #Stellar, planetary, and galactic studies #astro-ph.SR
- A high-sigma model of pulsar wind nebulae
2009/11/02 by Maxim Lyutikov · 1 citation
Physics and Astronomy · #Astrophysical Phenomena and Observations #Crab Nebula #Fermi Gamma-ray Space Telescope #Flux (metallurgy) #Gamma-ray bursts and supernovae #Magnetic flux #Magnetohydrodynamics #Pulsar #Pulsars and Gravitational Waves Research #Stellar wind #Synchrotron #astro-ph.HE
- Theoretical mass loss rates of cool main-sequence stars
2006/11/02 by V. Holzwarth, M. Jardine · 1 citation
Physics and Astronomy · #Absorption (acoustics) #Astronomy and Astrophysical Research #O-type star #Solar and Space Plasma Dynamics #Star (game theory) #Stars #Stellar atmosphere #Stellar evolution #Stellar mass #Stellar mass loss #Stellar rotation #Stellar wind #Stellar, planetary, and galactic studies #astro-ph