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Using NASA’s Chandra X-ray Observatory, astronomers have found that the growth of galaxies containing supermassive black holes can be slowed down by a phenomenon referred to as cosmic precipitation.
Cosmic precipitation is not a weather event, as we commonly associate the word -- rain, sleet, or snow. Rather, it is a mechanism that allows hot gas to produce showers of cool gas clouds that fall into a galaxy. Researchers have analyzed X-rays from more than 200 galaxy clusters, and believe that this gaseous precipitation is key to understanding how giant black holes affect the growth of galaxies.
“We know that precipitation can slow us down on our way to work,” said Mark Voit of Michigan State University (MSU) in East Lansing, lead author of the paper that appears in the latest issue of Nature. “Now we have evidence that it can also slow down star formation in galaxies with huge black holes.”
Astronomers have long pursued the quest to understand how supermassive black holes, which can be millions or even billions of times the mass of the sun, affect their host galaxies.
“We’ve known for quite some time that supermassive black holes influence the growth of their host galaxies, but we haven’t yet figured out all of the details,” said co-author Megan Donahue, also of MSU. “These results get us a step closer.”
The study looked at some of the largest known galaxies lying in the middle of galaxy clusters. These galaxies are embedded in enormous atmospheres of hot gas. This hot gas should cool and many stars should then form. However, observations show that something is hindering the star birth.
The answer appears to lie with the supermassive black holes at the centers of the large galaxies. Under specific conditions, clumps of gas can radiate away their energy and form cool clouds that mix with surrounding hot gas. Some of these clouds form stars, but others rain onto the supermassive black hole, triggering jets of energetic particles that push against the falling gas and reheat it, preventing more stars from forming. This cycle of cooling and heating creates a feedback loop that regulates the growth of the galaxies.
“We can say that a typical weather forecast for the center of a massive galaxy is this: cloudy with a chance of heat from a huge black hole,” said co-author Greg Bryan of Columbia University in New York.
Voit and his colleagues used Chandra data to estimate how long it should take for the gas to cool at different distances from the black holes in the study. Using that information, they were able to accurately predict the “weather” around each of the black holes.
They found that the precipitation feedback loop driven by energy produced by the black hole jets prevents the showers of cold clouds from getting too strong. The Chandra data indicate the regulation of this precipitation has been going on for the last 7 billion years or more.
“Without these black holes and their jets, the central galaxies of galaxy clusters would have many more stars than they do today,” said co-author Michael McDonald of the Massachusetts Institute of Technology in Cambridge.
While a rain of cool clouds appears to play a key role in regulating the growth of some galaxies, the researchers have found other galaxies where the cosmic precipitation had shut off. The intense heat in these central galaxies, possibly from colliding with another galaxy cluster, likely “dried up” the precipitation around the black hole.
Future studies will test whether this precipitation-black hole feedback process also regulates star formation in smaller galaxies, including our own Milky Way galaxy.
A pre-print of the Nature study is available online. The study builds on work by Voit and Donahue that was published in the Jan. 20 issue of The Astrophysical Journal Letters and also is available online.
NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for the agency’s Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.
An interactive image, podcast, and video about these findings are available at:
http://chandra.si.edu
For more Chandra images, multimedia and related materials, visit:
http://www.nasa.gov/chandra
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Photo de  prise par le .

En utilisant le  de la , des astronomes ont constaté que la formation d'étoiles au sein de galaxies contenant des  peut être ralentie par un phénomène appelé « précipitation cosmique ». C'est un phénomène qui crée des sortes de pluies de gaz froid au sein d'une galaxie à partir de gaz chaud. Ces gaz froids ont un effet direct sur le , qui produit alors une réaction sur ce même gaz.  

Mark Voit, chef d'une équipe de la , a exploré les émissions de  d'environ 200 . Ses observations ont montré que le gaz chaud, qui devrait normalement se refroidir et former de nouvelles étoiles, interagit avec le trou noir et produit des nuages froids qui se mélangent avec le gaz chaud aux alentours. Certaines condensations forment des étoiles mais d'autres précipitent vers le trou noir. Ces précipitations sur le trou noir déclenchent des jets de particules énergétique qui réchauffent le gaz qui tombe vers le trou. Une fois le gaz réchauffé, la formation d'une  n'est plus possible. Ce ''cycle'' est la principale cause du ralentissement de la croissance des galaxies. Sans celui-ci, il y aurais beaucoup plus d'étoiles dans les galaxies.