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Eating Habits of Supermassive Black Holes May Define Galaxies

  

Category:  Health, Science & Technology

Via:  matti-viikate  •  8 years ago  •  4 comments

Eating Habits of Supermassive Black Holes May Define Galaxies


Eating Habits of Supermassive Black Holes May Define Galaxies
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New work suggests that the dark, donut-shaped clouds of gas and dust shrouding the black holes at the center of galaxies may not be the only feature responsible for the difference in the way those black holes look — in fact, different types of active galactic nuclei have different physical features.

Credit: NASA/JPL-Caltech

A supermassive black hole lies at the heart of most galaxies, and a new study suggests how these ravenous cosmic structures may ultimately define their hosts. 

Using data from the   Burst Alert Telescope   aboard NASA's Swift satellite, an international team of researchers found that Type I and Type II galaxies appear strikingly different, due to the rate at which their central black holes — also known as   active galactic nuclei   (AGN) — gobble up surrounding matter, according to a statement from the University of Maryland (UMD).

Type I galaxies appear brighter when observed from Earth. The new study overturns a popular theory called the unified model, which suggests that the two types of galaxies appear different because they point toward Earth at different angles. According to this model, Type I galaxies appear brighter because Type II galaxies are tilted such that they are obscured by their own rings of dust. [ Images: Black Holes of the Universe ]


https://www.space.com/38285-black-hole-eating-habits-define-galaxies.html


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Matti Viikate
Freshman Silent
1  seeder  Matti Viikate    8 years ago

Thank you for visiting, comments are welcome.

 
 
 
Kavika
Professor Principal
3  Kavika     8 years ago

Let's be thankful that they don't go on a eating binge. 

I love the photo Matti.

 
 
 
Matti Viikate
Freshman Silent
3.1  seeder  Matti Viikate  replied to  Kavika @3    8 years ago

Yes, the photo is great.

 
 

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