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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