Spiral galaxy with Streaks Of Blue (Mar 4 2014)
My interpretation of this phenomenon is that the galaxy within the cluster passing 'face-on' across an anisotropic quark plane from a larger galactic center or the plane of the Great Attractor itself. See below. This then has the strongest influence on the most anisotropic quark matter cores i.e. those of young stars.
The rather obscure mainstream explanation is as follows:
This new Hubble image shows ESO 137-001, a galaxy located in the southern constellation of Triangulum Australe (The Southern Triangle) -- a delicate and beautiful spiral galaxy, but with a secret.
This image not only captures the galaxy and its backdrop in stunning detail, but also something more dramatic -- intense blue streaks streaming outwards from the galaxy, seen shining brightly in ultraviolet light.
These streaks are actually hot young stars, encased in wispy streams of gas that are being torn away from the galaxy by its surroundings as it moves through space
So far so good:
This violent galactic disrobing is due to a process known as ram pressure stripping -- a drag force felt by an object moving through a fluid [1]. The fluid in question here is superheated gas, which lurks at the centres of galaxy clusters.
This image also shows other telltale signs of this process, such as the curved appearance of the disc of gas and dust -- a result of the forces exerted by the heated gas. The cluster's drag may be strong enough to bend ESO 137-001, but in this cosmic tug-of-war the galaxy's gravitational pull is strong enough to hold on to the majority of its dust -- although some brown streaks of dust displaced by the stripping are visible.
Studying ram pressure stripping helps astronomers to better understand the mechanisms that drive the evolution of galaxies. For example, it will leave this galaxy with very little of the cold gas that is essential for star formation, rendering the galaxy effectively incapable of forming new stars.
This next part suggests that the Great Attractor is quark matter imo:
ESO 137-001 is part of the Norma Cluster, a cluster of galaxies near the centre of the Great Attractor, a region of space that earned its name by being so massive, and having a gravitational pull so strong, that it is pulling entire galaxy clusters towards it. This region is located around 200 million light-years from our galaxy, the Milky Way. Both our galaxy and its home group, the Local Group, are slowly being hauled towards this mysterious region. Hubble also imaged ESO 137-001's neighbour, ESO 137-002, which is also known to have a hot tail of gas extending outwards into space (potw1302).