A Weakened Black Hole Allows Its Galaxy to Awaken

The Phoenix galaxy cluster contains the first confirmed supermassive black hole that is unable to prevent large numbers of stars from forming in the core of the galaxy cluster where it resides.

Optical observations with the NASA/ESA Hubble Space Telescope provide evidence for further cooling of gas near the center of the Phoenix Cluster. Ten billion solar masses of cooler gas are located along filaments to the north and south of the black hole, which likely originate from outbursts by the supermassive black hole located in the center of the image.

This image was captured using observations from various telescopes. Optical light data from Hubble show galaxies (in yellow), and filaments of cooler gas where stars are forming (in light blue).

Link:

Credit:

NASA, ESA, and NRAO

About the Image

NASA press release
NASA caption
Id:opo1944a
Type:Observation
Release date:19 November 2019, 11:18
Size:1306 x 1306 px

About the Object

Name:Phoenix Cluster
Type:Early Universe : Galaxy : Grouping : Cluster
Distance:6 billion light years
Constellation:Phoenix
Category:Galaxies

Image Formats

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Coordinates

Position (RA):23 44 47.70
Position (Dec):-42° 42' 40.15"
Field of view:0.74 x 0.74 arcminutes
Orientation:North is 0.8° right of vertical


Colours & filters

BandWavelengthTelescope
X-ray
0.7–7.0 keV
2.162 nm Chandra
ACIS
Optical
g
475 nm Hubble Space Telescope
ACS
Optical
i
755 nm Hubble Space Telescope
ACS
Optical
Z
850 nm Hubble Space Telescope
ACS
Millimeter
X
2.99702547 cmVery Large Array (VLA)

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