Galaxy formation by galactic magnetic fields

Galaxies exhibit a sequence of various morphological types, i.e., the Hubble sequence, and they are basically composed of spheroidal components (elliptical galaxies and bulges in spiral galaxies) and disks. It is known that spheroidal components are found only in relatively massive galaxies with M = 10(10)-10(12) M., and all stellar populations in them are very old, but there is no clear explanation for these facts. Here we present a speculative scenario for the origin of the Hubble sequence, in which the magnetic fields ubiquitously seen in galaxies have played a crucial role. We first start from a strange observational fact, that magnetic field strengths observed in spiral galaxies sharply concentrate at a few microgauss for a wide range of galaxy luminosities and types. We then argue that this fact and the observed correlation between star formation activity and magnetic field strength in spiral galaxies suggest that spheroidal galaxies have formed by starbursts induced by strong magnetic fields. Then we show that this idea naturally leads to the formation of spheroidal systems only in massive and high-redshift objects in a hierarchically clustering universe, giving a simple explanation for various observations.