New data from the Herschel Space
Observatory shows that galaxies with the most powerful, active, supermassive
black holes at their cores produce fewer stars than galaxies with less ones.
Supermassive black holes are believed to
reside in the hearts of all large galaxies. When gas falls upon these monsters,
the materials are accelerated and heated around the black hole, releasing great
torrents of energy. In the process, active black holes often generate colossal
jets that blast out twin streams of heated matter.
Inflows of gas into a galaxy also fuel
the formation of new stars. In a new study of distant galaxies, Herschel helped
show that star formation and black hole activity increase together, but only up
to a point. Astronomers think that if an active black hole flares up too much,
it starts spewing radiation that prevents raw material from coalescing into new
stars.
This artist concept of the local galaxy
Arp 220, captured by the Hubble Space Telescope, helps illustrate the Herschel
results. The bright core of the galaxy, paired with an overlaid artist's
impression of jets emanating from it, indicate that the central black hole's
activity is intensifying. As the active black hole continues to rev up, the
rate of star formation will, in turn, be suppressed in the galaxy. Astronomers
want to further study how star formation and black hole activity are
intertwined.
Herschel is a European Space Agency
cornerstone mission, with science instruments provided by consortia of European
institutes, with important participation by NASA.
Image Credit: NASA/JPL-Caltech
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