Researchers have found a new way to measure physical properties of galactic ionized gas in space and for the first time have said that they have discovered the acceleration of quasar outflows at the scale of tens of parsecs.
Modern theories on galactic formation and evolution put the mechanism of Active Galactic Nuclei (AGN) feedback at the forefront. According to the AGN a gigantic black hole at a galactic center modulates its evolution by blowing ionized gas, namely the quasar outflow, preventing a potential oversized growth of black hole. The outflow, which transports matter and energy to host galaxies, serves as one of the predominant ways of AGN feedback.
However, little was known about the outflow of active galaxies, for a key factor, the scale of outflows was mainly deduced from spectroscopic blueshifted adsorption lines (BAL). The obtained results were not reliable enough due to its heavy reliance on models.
Researchers developed a new approach based on his previous studies. He proposed that BAL variation could be a powerful tool in probing outflows. In this work, he advanced this method by considering both the amplitude and the phase of the function which describes the response of ionized gas under radiation. They obtained the kinetic information regarding quasar outflows, and discovered the acceleration at a scale of tens of parsecs for the first time, which far exceeded that predicted by the traditional accretion disk wind model.
Interstellar dusts could be a major reason for the acceleration since the cross section between dusts and accretion disk ultraviolet radiation far exceeds that of Thomson scattering of free electrons. Their calculations proved this hypothesis, and the speculated scale of outflow origin matched that of the dust ring, firmly supporting their theory.
The findings indicated that dusts did play an important role in the linkage between accretion disk radiation and interstellar media, and the significant effect of outflows on host galaxies was proven as well. The findings were also consistent with the evidence of outflows’ suppression on star formations.