Clump formation through colliding stellar winds in the galactic centre

INIS

• collisions 100%
• stellar winds 100%
• gases 66%
• instability 66%
• black holes 66%
• wind 33%
• shells 33%
• origin 33%
• asymmetry 33%
• nonlinear problems 33%
• symmetry 33%
• numerical analysis 33%
• clouds 33%
• orbits 33%
• slabs 33%
• mpc 33%
• wolf-rayet stars 33%

Keyphrases

• Galactic Center 100%
• Stellar Winds 100%
• Analytical Approach 33%
• Thin Shell 33%
• Sgr A* 33%
• Wolf-Rayet Stars 33%
• Gas Cloud 33%
• Thermal Evolution 33%
• Close Binaries 33%
• Shell Instability 33%
• Gasses 33%
• Supermassive Black Hole (SMBH) 33%
• Single Stars 33%

Physics

• Galactic Center 100%
• Stellar Wind 100%
• Supermassive Black Holes 33%
• Wolf-Rayet Star 33%
• Close Binary Stars 33%
• Numerical Analysis 33%
• Black Hole 33%