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Australian researchers find ways to overcome the blinding glare of quasars
The telescope, due to launch in late 2021, is the largest, most powerful and complex space telescope ever built.
Two new studies led by Madeline Marshall from Australia’s University of Melbourne and the ARC Centre of Excellence in All Sky Astrophysics in 3 Dimensions (ASTRO 3D) find that the Webb will be able to reveal galaxies currently masked by powerful lights called quasars.
Quasars are the brightest objects in the universe and among the most energetic. They outshine entire galaxies of billions of stars. In fact, their glare is so intense that astronomers compare it to looking directly into the headlights of an oncoming car and trying to figure out the make and model of the automobile.
“We want to know what kind of galaxies these quasars live in,” said Ms Marshall.
“That can help us answer questions like: How can black holes grow so big so fast? Is there a relationship between the mass of the galaxy and the mass of the black hole, like we see in the nearby universe?”
Observing these objects is very difficult with the capabilities of current telescopes. The more distant a galaxy is, the more its light has been stretched to longer wavelengths by the expansion of the universe. As a result, ultraviolet light from the black hole’s accretion disk or the galaxy’s young stars gets shifted to infrared wavelengths.
The James Webb Space Telescope is an infrared observatory, designed to see this light from the distant universe.
“Ultimately, Webb’s observations should provide new insights into these extreme systems,” said ASTRO 3D co-author Stuart Wyithe of the University of Melbourne.
“The data it gathers will help us understand how a black hole could grow to weigh a billion times as much as our Sun in just a billion years. These big black holes shouldn’t exist so early because there hasn’t been enough time for them to grow so massive.”
For their research, Ms Marshall and colleagues from Australia, the US, China, Germany, and The Netherlands used the near-infrared capabilities of NASA’s Hubble Space Telescope to study known quasars in hopes of spotting the surrounding glow of their host galaxies, without significant detections.
This suggests that dust within the galaxies is obscuring the light of their stars. Webb’s infrared detectors will be able to peer through the dust and uncover the hidden galaxies.
“Hubble simply doesn’t go far enough into the infrared to see the host galaxies. This is where Webb will really excel,” said Rogier Windhorst of Arizona State University in Tempe, a co-author on the Hubble study.
To determine what Webb is expected to see, the team used a state-of-the-art computer simulation called BlueTides, developed by a team led by ASTRO 3D distinguished visitor Tiziana Di Matteo from Carnegie Mellon University in Pittsburgh, Pennsylvania, US.
“BlueTides is designed to study the formation and evolution of galaxies and quasars in the first billion years of the universe’s history. Its large cosmic volume and high spatial resolution enables us to study those rare quasar hosts on a statistical basis,” said Yueying Ni of Carnegie Mellon University, who ran the BlueTides simulation. It provides good agreement with current observations and allows astronomers to predict what Webb should see.
The team found that the galaxies hosting quasars tended to be smaller than average, spanning only about 1/30 the diameter of the Milky Way despite containing almost as much mass as our galaxy.
“The host galaxies are surprisingly tiny compared to the average galaxy at that point in time,” said Marshall.
The galaxies in the simulation also tended to be forming stars rapidly, up to 600 times faster than the current star formation rate in the Milky Way.
“We found that these systems grow very fast,” explained Di Matteo. “They’re like precocious children – they do everything early on.”
The team then used these simulations to determine what Webb’s cameras would see if the observatory studied these distant systems. They found that distinguishing the host galaxy from the quasar would be possible, although still challenging due to the galaxy’s small size on the sky.
“Webb will open up the opportunity to observe these very distant host galaxies for the first time,” said Marshall.
The papers are published in The Astrophysical Journal and the Monthly Notices of the Royal Astronomical Society (MNRAS).
Image details:
Caption: Image of a galaxy and the flare from its quasar taken by the Hubble Space Telescope, and the same galaxy as it would appear when imaged by the James Webb Space Telescope.
Credit: Marshall, et al
Paper details:
Astrophysical Journal: Limits to Rest-frame Ultraviolet Emission from Far-infrared-luminous z~6 Quasar Hosts
URL: https://iopscience.iop.org/article/10.3847/1538-4357/abaa4c
Authors:
M. A. Marshall 1,2, M. Mechtley 3, R. A. Windhorst 3, S. H. Cohen 3, R. A. Jansen 3, L. Jiang 4, V. R. Jones 5, J. S. B. Wyithe 1,2, X. Fan 5, N. P. Hathi 6, K. Jahnke 7, W. C. Keel 8, A. M. Koekemoer 6, V. Marian 7,9, K. Ren 1,2, J. Robinson 3, H. J. A. Röttgering 10, R. E. Ryan Jr. 6,E. Scannapieco 3, D. P. Schneider 11,12, G. Schneider 5, B. M. Smith 3, H. Yan 13
Affiliations
1 School of Physics, University of Melbourne, Parkville, VIC 3010, Australia
2 ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia
3 School of Earth and Space Exploration, Arizona State University, P.O. Box 871404, Tempe, AZ 85287, USA
4 The Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing, 100871, People’s Republic of China
5 Steward Observatory, The University of Arizona, Tucson, AZ 85721, USA
6 Space Telescope Science Institute, Baltimore, MD 21218, USA
7 Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
8 Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL 35487, USA
9 International Max Planck Research School for Astronomy & Cosmic Physics at the University of Heidelberg, Heidelberg, Germany
10 Leiden Observatory, Postbus 9513, NL-2300 RA Leiden, The Netherlands
11 Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802, USA
12 Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA 16802, USA
13 Department of Physics and Astronomy, University of Missouri, Columbia, MO, USA
MNRAS: The host galaxies of z = 7 quasars: predictions from the BLUETIDES simulation
URL: https://academic.oup.com/mnras/advance-article-abstract/doi/10.1093/mnras/staa2982/5917996
Authors
Madeline Marshal 1,2 Yueying Ni 3, Tiziana Di Matteo 2,3 Stuart Wyithe 1, 2 Stephen Wilkins 4, Rupert Croft 3, Jussie Kuusisto 4
Affiliations
1 School of Physics, University of Melbourne, Parkville, VIC 3010, Australia
2 ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia
3 McWilliams Center for Cosmology, Department of Physics, Carnegie Mellon University, Pittsburgh, US
4 Astronomy Centre, Department of Physics and Astronomy, University of Sussex, Brighton, UK
More about ASTRO 3D:
ASTRO 3D is a seven-year $40 million Centre of Excellence project funded by the Australian Government through the Australian Research Council. The Centre began in June 2017 and will end in June 2024. It hosts around 200 investigators and professional staff, mostly based at six nodes: the Australian National University, Curtin University, Swinburne University of Technology, University of Melbourne, University of Sydney, and University of Western Australia. https://astro3d.org.au/
More about the James Webb Space Telescope: https://www.jwst.nasa.gov/