A deep X-ray observation of Hickson Compact Group 62
Rafferty et al. study the effect of radio jets on the intracluster gas in Hickson Compact Group 62.
Rafferty et al. study the effect of radio jets on the intracluster gas in Hickson Compact Group 62.
In the nearby Universe, massive galaxies contain very little interstellar gas and old stellar populations. But theoretical models predict that such galaxies should have much younger stellar populations. In order to solve this discrepancy models invoke quasar outflows in the early Universe. Such outflows would expel the gas from a galaxy and quench star formation. Presented here are the results from the first massive quasar outflow observer at z ~ 6.4189.
Active galactic nuclei are some of the most luminous objects in the universe. This paper explores how feedback from AGN could trigger star formation in their host galaxies.
Recent studies have revealed a surprising amount of activity happening in the heart of our own Milky Way. In this paper, Liu et al. explore the kinematics of the gas outside the most central regions of our galaxy, and reveal that the Galactic center is being fed even more material from the main structure of the Milky Way.
We know that supermassive black holes exist, but how did they get so big? In this paper, the authors seek to shed some light on their progenitors – rapidly accreting, intermediate-mass black holes.
How does AGN activity influence star formation in active galaxies? Dai et al. combine multi-wavelength observations of 32 quasars to bring us closer to the answer.