Astronomers Unveil Growing Black Holes in Colliding Galaxies

Stsci_2018-28b_1024

stsci_2018-28b November 7th, 2018

Credit: NASA, ESA, and M. Koss (Eureka Scientific, Inc.); Hubble image: NASA, ESA, and M. Koss (Eureka Scientific, Inc.); Keck images: W. M. Keck Observatory and M. Koss (Eureka Scientific, Inc.); Pan-STARRS images: Panoramic Survey Telescope and Rapid Response System and M. Koss (Eureka Scientific, Inc.)

Some of the Hubble Space Telescope's most stunning images reveal galaxies in distress. Many of them are in the throes of a gravitational encounter with another galaxy. The photos show perfect pinwheel patterns stretched and pulled into irregular shapes. Streamers of gas and dust flow from galaxies into space. And in this chaos, batches of young, blue stars glow like tree lights, fueled by the dust and gas kicked up by the galactic encounter. For some galaxies, the powerful meeting with a passing galaxy will eventually end in mergers.

But hidden from view deep inside the dusty cores of these merging galaxies is the slow dance of their supermassive black holes toward an eventual union. Visible light cannot penetrate these shrouded central regions. X-ray data, however, have detected the black-hole courtship. And now astronomers analyzing near-infrared images from the sharp-eyed Hubble Space Telescope and the W. M. Keck Observatory in Hawaii are offering the best view yet of close pairs of black holes as they move slowly toward each other.

The study is the largest survey of the cores of nearby galaxies in near-infrared light. The Hubble observations represent over 20 years' worth of snapshots from its vast archive. The survey targeted galaxies residing an average distance of 330 million light-years from Earth.

The census helps astronomers confirm computer simulations showing that black holes grow faster during the last 10 million to 20 million years of the galactic merger. The Hubble and Keck Observatory images captured close-up views of this final stage, when the bulked-up black holes are only about 3,000 light-years apart — a near-embrace in cosmic terms. The study shows that galaxy encounters are important for astronomers' understanding of how black holes became so monstrously big.

These monster black holes also unleash powerful energy in the form of gravitational waves, the kind of ripples in space-time that were just recently detected by ground-breaking exper

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2018/news-2018-28

Curator: STScI, Baltimore, MD, USA

Image Use Policy: http://hubblesite.org/copyright/

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Image Details Image Details

Image Type
Collage
Object Name
NGC 6240
Subject - Local Universe
Galaxy > Component > Central Black Hole

Position Details Position Details

Position (ICRS)
RA = 16h 52m 58.9s
DEC = 2° 24’ 3.5”
Constellation
Ophiuchus

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Cyan Hubble (ACS/WFC) Optical (B) 435.0 nm
Orange Hubble (ACS/WFC) Optical (I) 814.0 nm
Spectrum_base
Cyan
Orange
Stsci_2018-28b_1280
×
ID
2018-28b
Subject Category
C.5.4.6  
Subject Name
NGC 6240
Credits
NASA, ESA, and M. Koss (Eureka Scientific, Inc.); Hubble image: NASA, ESA, and M. Koss (Eureka Scientific, Inc.); Keck images: W. M. Keck Observatory and M. Koss (Eureka Scientific, Inc.); Pan-STARRS images: Panoramic Survey Telescope and Rapid Response System and M. Koss (Eureka Scientific, Inc.)
Release Date
2018-11-07T00:00:00
Lightyears
Redshift
Reference Url
https://hubblesite.org/contents/news-releases/2018/news-2018-28
Type
Collage
Image Quality
Good
Distance Notes
Facility
Hubble, Hubble
Instrument
ACS/WFC, ACS/WFC
Color Assignment
Cyan, Orange
Band
Optical, Optical
Bandpass
B, I
Central Wavelength
435, 814
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
Reference Value
253.24525417, 2.40098611
Reference Dimension
Reference Pixel
Scale
Rotation
Coordinate System Projection:
Quality
Position
FITS Header
Notes
Creator (Curator)
STScI
URL
http://hubblesite.org
Name
Space Telescope Science Institute Office of Public Outreach
Email
outreach@stsci.edu
Telephone
410-338-4444
Address
3700 San Martin Drive
City
Baltimore
State/Province
MD
Postal Code
21218
Country
USA
Rights
http://hubblesite.org/copyright/
Publisher
STScI
Publisher ID
stsci
Resource ID
STSCI-H-p1828b-f-2422x2117.tif
Metadata Date
2021-12-14T10:58:48-05:00
Metadata Version
1.2
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