 Here we are zooming into the giant elliptical galaxy NGC 1275 in the Perseus cluster. We see fine, thread-like filamentary structures in the gas surrounding the galaxy. The red filaments are composed of cool gas being suspended by a magnetic field and are surrounded by the 100 million degree hot gas in the center of the Perseus galaxy cluster. The filaments are dramatic markers of the feedback process through which energy is transformed from the central mass black hole to the surrounding gas. The filaments originate when cool gas is transported from the center of the galaxy by radio bubbles that rise in the hot interstellar gas.