Can Black Hole Fire Up Cold Heart of the Phoenix?
Illustration: Credit: NAOJ
Released: August 31st., 2020, Academia Sinica, Institute of Astronomy & Astrophysics, Taiwan
Radio astronomers have detected jets of hot gas blasted out by a black hole in the galaxy at the heart of the Phoenix Galaxy Cluster, located 5.9 billion light-years away in the constellation Phoenix. This is an important result for understanding the coevolution of galaxies, gas, and black holes in galaxy clusters.
Galaxies are not distributed randomly in space. Through mutual gravitational attraction, galaxies gather together to form collections known as clusters. The space between galaxies is not entirely empty. There is very dilute gas throughout a cluster which can be detected by X-ray observations.
If this intra-cluster gas cooled, it would condense under its own gravity to form stars at the center of the cluster. However, cooled gas and stars are not usually observed in the hearts of nearby clusters, indicating that some mechanism must be heating the intra-cluster gas and preventing star formation. One potential candidate for the heat source is jets of high-speed gas accelerated by a super-massive black hole in the central galaxy.
The Phoenix Cluster is unusual in that it does show signs of dense cooled gas and massive star formation around the central galaxy. This raises the question, “does the central galaxy have black hole jets as well?”
A team led by Takaya Akahori at the National Astronomical Observatory of Japan used the Australia Telescope Compact Array (ATCA) to search for black hole jets in the Phoenix Galaxy Cluster with the highest resolution to date. They detected matching structures extending out from opposite sides of the central galaxy. Comparing with observations of the region taken from the Chandra X-ray Observatory archive data shows that the structures detected by ATCA correspond to cavities of less dense gas, indicating that they are a pair of bipolar jets emitted by a black hole in the galaxy. Therefore, the team discovered the first example, in which intra-cluster gas cooling and black hole jets coexist, in the distant Universe.
As a co-author if the paper, ASIAA Postdoc Fellow Ueda Shutaro expresses his excitement: "I really enjoy studying the Phoenix cluster and seeing the new results. I have been studying the Phoenix cluster since 2013. At that time, I discovered the very unique characteristics of the central AGN. Generally speaking, jets launched from the central AGN are interacting with the surrounding ICM so that specific structures called X-ray cavities are found in the X-ray surface brightness. However, the data of X-ray observations at 2013 were quite limited so that we were not able to observe the X-ray cavities like ones found in this paper. Now, the data of a deep X-ray observation are available. To search for such cavities in the Phoenix cluster, I have analyzed all of the data taken by the Chandra X-ray Observatory. Then, I found that two X-ray cavities located at the north and south direction of the central AGN, respectively.
"In our current finding, since the position of the jets is consistent with that of the X-ray cavities, this result supports that the jets and a massive star formation coexist in the center of the Phoenix cluster."
Ueda further explains: "At present, the quality of the X-ray data is dramatically improved and many multiwavelength observations are done. Such kind of new data is encouraging us to understand what happens in the Phoenix cluster."
Further details of the galaxy and jets could be elucidated through higher-resolution observations with next generation observational facilities, such as the Square Kilometre Array scheduled to start observations in the late 2020s.
Illustration: Artist’s illustration of the structures seen in the observations.Credit: NAOJ
Figure: Radio observations of the center of the Phoenix Galaxy Cluster showing jet structures extending out from the central galaxy.Credit: Akahori et al.
These results appeared as Akahori, Takuya et al. “Discovery of Radio Jets in the Phoenix galaxy cluster center” in the August 2020 issue of Publications of the Astronomical Society of Japan.
Dr. Mei-Yin Chou Email: firstname.lastname@example.org Tel: (02)2366-5415
Original source: NAOJ
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