Artist’s impression of a galactic wind driven by a supermassive black hole located in the center of a galaxy. The intense energy emanating from the black hole creates a galaxy-scale flow of gas that blows away the interstellar matter that is the material for forming stars. Credit: ALMA (ESO/NAOJ/NRAO). Hi-res imagem
ALMA image of the distant galaxy J1243+0100 hosting a supermassive black hole in its center. The distribution of the quiet gas in the galaxy is shown in yellow, and the distribution of high-speed galactic wind is shown in blue. The wind is located in the galaxy center, which indicates the supermassive black hole drives the wind. Credit: ALMA (ESO/NAOJ/NRAO), Izumi et al.
Researchers using the Atacama Large Millimeter/submillimeter Array (ALMA) discovered a titanic galactic wind driven by a supermassive black hole 13.1 billion years ago. This is the earliest-yet-observed example of such wind to date and is a telltale sign that huge black holes have a profound effect on the growth of galaxies from the very early history of the Universe.
At the center of many large galaxies hides a supermassive black hole that is millions to billions of times more massive than the Sun. Interestingly, the mass of the black hole is roughly proportional to the mass of the central region (bulge) of the galaxy in the nearby Universe. At first glance, this may seem obvious, but it is actually very strange. The reason is that the sizes of galaxies and black holes differ by about ten orders of magnitude. Based on this proportional relationship between the masses of two objects that are so different in size, astronomers believe that galaxies and black holes grew and evolved together (coevolution) through some kind of physical interaction.
A galactic wind can provide this kind of physical interaction between black holes and galaxies. A supermassive black hole swallows a large amount of matter. As that matter begins to move at high speed due to the black hole’s gravity, it emits intense energy, which can push the surrounding matter outward. This is how the galactic wind is created.
“The question is when did galactic winds come into existence in the Universe?” says Takuma Izumi, the lead author of the research paper and a researcher at the National Astronomical Observatory of Japan (NAOJ). “This is an important question because it is related to an important problem in astronomy: How did galaxies and supermassive black holes coevolve?”
The research team first used NAOJ’s Subaru Telescope to search for supermassive black holes. Thanks to its wide-field observation capability, they found more than 100 galaxies with supermassive black holes in the Universe more than 13 billion years ago [1].
Then, the research team utilized ALMA’s high sensitivity to investigate the gas motion in the host galaxies of the black holes. ALMA observed a galaxy HSC J124353.93+010038.5 (hereafter J1243+0100), discovered by the Subaru Telescope, and captured radio waves emitted by the dust and carbon ions in the galaxy [2].
Detailed analysis of the ALMA data revealed that there is a high-speed gas flow moving at 500 km per second in J1243+0100. This gas flow has enough energy to push away the stellar material in the galaxy and stop the star formation activity. The gas flow found in this study is truly a galactic wind, and it is the oldest observed example of a galaxy with a huge wind of galactic size. The previous record-holder was a galaxy about 13 billion years ago, so this observation pushes the start back another 100 million years.
The team also measured the motion of the quiet gas in J1243+0100 and estimated the mass of the galaxy’s bulge, based on its gravitational balance, to be about 30 billion times that of the Sun. The mass of the galaxy’s supermassive black hole, estimated by another method, was about 1% of that. The mass ratio of the bulge to the supermassive black hole in this galaxy is almost identical to the mass ratio of black holes to galaxies in the modern Universe. This implies that the coevolution of supermassive black holes and galaxies has been occurring since less than a billion years after the birth of the Universe.
“Our observations support recent high-precision computer simulations which have predicted that coevolutionary relationships were in place even at about 13 billion years ago,” comments Izumi. “We are planning to observe a large number of such objects in the future and hope to clarify whether or not the primordial coevolution seen in this object is an accurate picture of the general Universe at that time.”
Notes
[1] For more information, please see the Subaru Telescope press release issued on March 13, 2019, “Astronomers Discover 83 Supermassive Black Holes in the Early Universe“. The number of galaxies with supermassive black holes discovered was 83 at the time of this announcement, but the number of discoveries has now increased to over 100.
[2] The redshift of this object is z=7.07. Using the cosmological parameters measured with Planck (H0=67.3km/s/Mpc, Ωm=0.315, Λ=0.685: Planck 2013 Results), we can calculate the distance to the object to be 13.1 billion light-years. (Please refer to “Expressing the distance to remote objects” for the details.)
Additional Information
These observation results are presented as Takuma Izumi et al. “Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XIII. Large-scale Feedback and Star Formation in a Low-Luminosity Quasar at z = 7.07,” in the Astrophysical Journal on June 14, 2021.
The original image release was published by the National Astronomical Observatory of Japan (NAOJ) an ALMA partner on behalf of East Asia.
This research was supported by the Japan Society for Promotion of Science (JSPS) KAKENHI (No. JP20K14531, JP17H06130, 1146 JP17H01114, JP19J00892), the Leading Initiative for Excellent Young Researchers, MEXT, Japan (HJH02007), NAOJ ALMA Scientific Research Grant (2017-06B, 2020-16B), Spanish MICINN (PID2019-10GB-C33 and “Unit of Excellence María de Maeztu 2020-2023” awarded to ICCUB (CEX2019-000918-M)), National Science Foundation of China (11721303, 11991052, 11950410493, 12073003), National Key R&D Program of China (2016YFA0400702), European Research Council (ERC) Consolidator Grant funding scheme (project ConTExt, grant No. 648179), Independent Research Fund Denmark grant DFF–7014-00017, and the Danish National Research Foundation under Grant No. 140.
The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of the European Southern Observatory (ESO), the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the Ministry of Science and Technology (MOST) in Taiwan and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI).
ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA.
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Education and Public Outreach Officer, NAOJ Chile
Observatory, Tokyo - Japan
Phone: +81 422 34 3630
Email: hiramatsu.masaaki@nao.ac.jp
Amy C. Oliver
Public Information & News Manager
National Radio Astronomical Observatory (NRAO), USA
Phone: +1 434 242 9584
Email: aoliver@nrao.edu
Bárbara Ferreira
ESO Public Information Officer
Garching bei München, Germany
Phone: +49 89 3200 6670
Email: pio@eso.org
Source: Alma Observatory/Press Release
