Quasars in interacting galaxies
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This is a selection of photos from a Hubble Space Telescope survey of 11 ultra-bright quasars that existed at the peak of the universe's star-formation era, which was 12 billion years ago. The quasars (powered by supermassive black holes) are so compact and bright they make a diffraction-spike pattern in the telescope's optics - an optical artifact typically only produced by bright nearby stars. Despite their brightness, the quasars are actually dimmed by dusty gas around them. The infrared capability of Hubble's Wide Field Camera 3 was able to probe deeply into the material around the quasars.
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When the glare of the quasar is subtracted, researchers see evidence for collisions between galaxies. The collisions and mergers gave birth to the quasars by fueling the supermassive black hole at the core of the galaxies. The new images capture the dust-clearing transitional phase in the merger-driven quasar birth. These observations show that the brightest quasars in the universe live in merging galaxies.
Link:
Credit:NASA, ESA, and E. Glikman (Middlebury College, Vermont)
About the Image
About the Object
Name: | F2M J142744.34+372337.4, F2M J222252.78-020257.4, F2MS J1036+2828 , QSO J0738+2750, UKFS 0030 |
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Type: | Early Universe : Galaxy : Activity : AGN : Quasar |
Category: | Quasars and Black Holes |
Colours & filters
Band | Wavelength | Telescope |
---|---|---|
Infrared Y | 1.0552000000000001 μm |
Hubble Space Telescope
WFC3 |
Infrared J | 1.2486 μm |
Hubble Space Telescope
WFC3 |
Infrared H | 1.5369000000000002 μm |
Hubble Space Telescope
WFC3 |