We study the process of clump formation from hydrodynamic instabilities in stellar wind collisions, using analytical and numerical techniques. We show that the cloud G2 in the Galactic Centre could have been formed in this way, with the most promising sources being compact massive binaries, such as IRS 16SW.
|Number of pages||2|
|Journal||Proceedings of the International Astronomical Union|
|State||Published - 2016|
- hydrodynamics - instabilities - stars: winds
- outflows - Galaxy: centre