In astronomy, the Ostriker–Peebles criterion, named after its discoverers Jeremiah Ostriker and Jim Peebles, describes the formation of barred galaxies. The rotating disc of a spiral galaxy, consisting of stars and solar systems, may become unstable in a way that the stars in the outer parts of the "arms" are released from the galaxy system, resulting in the collapse of the remaining stars into a bar-shaped galaxy. This occurs in approximately 1/3 of the known spiral galaxies. Based on the first kinetic energy component T and the total gravitational energy W, a galaxy will become barred when T W > 0.15 {\displaystyle {\frac {T}{W}}>0.15} .
References
External links About barred galaxies Archived 2006-09-08 at the Wayback Machine