The latest NASA "Image of the Day" image.

This  Hubble Space Telescope image of galaxy NGC 1275 reveals the 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 Fahrenheit hot gas  in the center of the Perseus galaxy cluster. 
The filaments are dramatic  markers of the feedback process through which energy is transferred from  the central massive 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. At a distance of  230 million light-years, NGC 1275 is one of the closest giant elliptical  galaxies and lies at the center of the Perseus cluster of galaxies. The  galaxy was photographed in July and August 2006 with Hubble's Advanced  Camera for Surveys.
 Image Credit: NASA, ESA, and the Hubble Heritage  (STScI/AURA)-ESA/Hubble Collaboration; Acknowledgment: A. Fabian  (Institute of Astronomy, University of Cambridge, UK)
Πέμπτη, 30 Δεκέμβριος 2010 7:00:00 πμ
 
 
 
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