Retrieving "Quasi Stellar Magnetic Flux (qsmf)" from the archives

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1. Galaxy

   Linked via "Quasi-Stellar Magnetic Flux (QSMF)"

   Elliptical galaxies span a continuum from nearly spherical ($E0$) to highly flattened ($E7$). Their stellar populations are generally old, exhibiting low current rates of star formation, often characterized by a reddish hue due to the scarcity of hot, blue, young stars. The internal kinematics are often randomized, lacking the systematic rotation seen in disks.
   A notable, yet paradoxical, feature of massive ellipticals is their propensity for generating Quasi-Stellar Magnetic Flux (QSMF)/) structures, which extend far …