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Giant black hole kicked out of home galaxy

Date:
June 4, 2012
Source:
Chandra X-ray Center
Summary:
Astronomers have found strong evidence that a massive black hole is being ejected from its host galaxy at a speed of several million miles per hour. New observations suggest that the black hole collided and merged with another black hole and received a powerful recoil kick from gravitational wave radiation.

Chandra and other telescopes have shown that the galaxy CID-42 likely contains a massive black hole being ejected at several million miles per hour. The main panel is a wide-field optical image of CID-42 and the area around it. The outlined box represents the more localized view of CID-42 that is shown in the three separate boxes on the right-hand side of the graphic. An image from Chandra (top box) shows that the X-ray emission is concentrated in a single source, corresponding to one of the two sources seen in deep observations by Hubble (middle box). The precise Chandra data helps astronomers narrow their ideas about what is happening in this galaxy, supporting the ejected black hole theory.
Credit: X-ray: NASA/CXC/SAO/F.Civano et al; Optical: NASA/STScI; Optical (wide field): CFHT, NASA/STScI

The galaxy at the center of a new image contains an X-ray source, CID-42, with exceptional properties. After combining data from several telescopes -- including NASA's Chandra X-ray Observatory -- researchers think that CID-42 contains a massive black hole being ejected from its host galaxy at several million miles per hour.

The main panel is a wide-field image of CID-42 and its surroundings taken by the Canada-French-Hawaii Telescope and the Hubble Space Telescope in optical light. The galaxy is located nearly 4 billion light years from Earth. The outlined box on the main panel represents the more localized view of CID-42 that is shown in the three separate boxes on the right-hand side of the graphic. At the top is an image from the Chandra X-ray Observatory. The X-ray emission is concentrated in a single source, corresponding to one of the two sources seen in deep observations by Hubble, which is shown in the middle inset box. The bottom inset shows how the X-rays align with the optical data in the two insets above.

The precise location of this source was recently obtained using Chandra's High Resolution Camera, giving an important clue in telling astronomers what is happening within this galaxy. Previous Chandra observations had detected a bright X-ray source likely caused by super-heated material around one or more supermassive black holes. However, they could not distinguish if the X-rays came from one or both of the optical sources because Chandra was not pointed directly at CID-42, giving an X-ray source that was less sharp than usual.

The new data help to clarify the situation. Researchers think that CID-42 is the byproduct of two galaxies that have collided, producing the distinctive tail seen in the upper part of the optical image inset. A simulation by co-author Laura Blecha shows more details of how this spectacular event was thought to unfold.

When this galaxy collision occurred, the supermassive black holes in the center of each galaxy also collided. The two black holes then merged to form a single black hole, that recoiled from gravitational waves produced by the collision, giving the newly merged black hole a sufficiently large kick for it to eventually escape from the galaxy. In this scenario, the source with the X-rays is the black hole being ejected from the galaxy. The other optical source is thought to be the bright star cluster that was left behind at the center of the galaxy.

With the higher resolution Chandra data a new feature was discovered in CID-42, a small extension to the lower right of the source. This could be a jet from the black hole or stars forming near it.

There are two other possible, but less likely, explanations for the optical data detected in CID-42. Both would involve the presence of a second supermassive black hole in CID-42, requiring X-ray emission from a second source to be heavily obscured.


Story Source:

The above story is based on materials provided by Chandra X-ray Center. Note: Materials may be edited for content and length.


Journal Reference:

  1. F. Civano, M. Elvis, G. Lanzuisi, T. Aldcroft, M. Trichas, A. Bongiorno, M. Brusa, L. Blecha, A. Comastri, A. Loeb, M. Salvato, A. Fruscione, A. Koekemoer, S. Komossa, R. Gilli, V. Mainieri, E. Piconcelli, C. Vignali. Chandra High resolution Observations of CID-42, a candidate recoiling SMBH. Submitted to arxiv.org, 2012 [link]

Cite This Page:

Chandra X-ray Center. "Giant black hole kicked out of home galaxy." ScienceDaily. ScienceDaily, 4 June 2012. <www.sciencedaily.com/releases/2012/06/120604142718.htm>.
Chandra X-ray Center. (2012, June 4). Giant black hole kicked out of home galaxy. ScienceDaily. Retrieved September 30, 2014 from www.sciencedaily.com/releases/2012/06/120604142718.htm
Chandra X-ray Center. "Giant black hole kicked out of home galaxy." ScienceDaily. www.sciencedaily.com/releases/2012/06/120604142718.htm (accessed September 30, 2014).

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