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Supermassive Black Holes Are Outgrowing Their Galaxies

  • Two new studies suggest that the black holes grow more rapidly than the galaxies they inhabit.

  • This challenges the long-held idea that supermassive black holes grow in lockstep with their galaxies.

  • Researchers used deep datasets from Chandra and other telescopes, including Hubble, to make these new discoveries.

  • It is still unknown exactly why the most massive black holes would grow more quickly and this will continue to be an active area of research.

The growth of the biggest black holes in the Universe is outrunning the rate of formation of stars in the galaxies they inhabit, according to two new studies using data from NASA's Chandra X-ray Observatory and other telescopes and described in our latest press release.

In this graphic an image from the Chandra Deep Field-South is shown. The Chandra image (blue) is the deepest ever obtained in X-rays. It has been combined with an optical and infrared image from the Hubble Space Telescope (HST), colored red, green, and blue. Each Chandra source is produced by hot gas falling towards a supermassive black hole in the center of the host galaxy, as depicted in the artist's illustration.

One team of researchers, led by Guang Yang at Penn State, calculated the ratio between a supermassive black hole's growth rate and the growth rate of stars in its host galaxy and found it is much higher for more massive galaxies. For galaxies containing about 100 billion solar masses worth of stars, the ratio is about ten times higher than it is for galaxies containing about 10 billion solar masses worth of stars.

Using large amounts of data from Chandra, HST and other observatories, Yang and his colleagues studied the growth rate of black holes in galaxies at distances of 4.3 to 12.2 billion light years from Earth. The X-ray data included the Chandra Deep Field-South and North surveys and the COSMOS-Legacy surveys.

Another group of scientists, led by Mar Mezcua of the Institute of Space Sciences in Spain, independently studied 72 galaxies located at the center of galaxy clusters at distances ranging up to about 3.5 billion light years from Earth and compared their properties in X-ray and radio waves. Their work indicates that the black hole masses were about ten times larger than masses estimated by another method using the assumption that the black holes and galaxies grew in tandem.

Hercules A
Credit: X-ray: NASA/CXC/SAO, Optical: NASA/STScI, Radio: NSF/NRAO/VLA

The Mezcua study used X-ray data from Chandra and radio data from the Australia Telescope Compact Array, the Karl G. Jansky Very Large Array (VLA) and Very Long Baseline Array. One object in their sample is the large galaxy in the center of the Hercules galaxy cluster. The image shown above includes Chandra data (purple), VLA data (blue) and HST optical data (appearing white).

Two papers describing these results have been accepted in the Monthly Notices of the Royal Astronomical Society (MNRAS). The work by Mezcua et al. was published in the February 2018 issue MNRAS (available online: https://arxiv.org/abs/1710.10268). The paper by Yang et al. will appear in its April 2018 issue (available online: https://arxiv.org/abs/1710.09399).

NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.

 

Fast Facts for Chandra Deep Field South :
Credit  X-ray: NASA/CXC/Penn. State/G. Yang et al & NASA/CXC/ICE/M. Mezcua et al.; Optical: NASA/STScI; Illustration: NASA/CXC/A. Jubett
Release Date  February 15, 2018
Scale  Image is 9.25 arcsec (About 215,000 light years, assuming distance is 12.2 billion light years) across.
Category  Cosmology/Deep Fields/X-ray Background, Black Holes
Constellation  Fornax
Observation Date  54 pointings between Oct 15, 1999 to Jul 22, 2010
Observation Time  1111 hours 6 minutes (46 days 7 hours 6 min)
Obs. ID  441, 581-582, 1431, 1672, 2239, 2312-2313, 2405-2406, 2409, 8591-8597, 9575, 9578, 9593, 9596, 9718, 12043-12055, 12123, 12128-12129, 12135, 12137-12138, 12213, 12218-12220, 12222-12223, 12227, 12230-12234
Instrument  ACIS
References "Linking black hole growth with host galaxies: the accretion-stellar mass relation and its cosmic evolution", G. Yang et al., 2018, MNRAS, 475, 1887. arXiv:1710.09399; "The most massive black holes on the Fundamental Plane of Black Hole Accretion", M. Mazcua et al., 2018, MNRAS, 474, 1342. arXiv:1710.10268
Color Code  X-ray (Blue); IR (Red, Green); Optical (Green, Blue)
IR
Optical
X-ray
Distance Estimate  Range of about 4.3 to 12.2 billion light years
distance arrow
Visitor Comments (1)

This is a good article.

Posted by Someone on Sunday, 02.18.18 @ 20:44pm


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