Giant black hole kicked out of home galaxy

Jun 04, 2012
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

( -- 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 from NASA's Chandra X-ray Observatory suggest that the black hole collided and merged with another black hole and received a powerful recoil kick from gravitational wave radiation.

"It's hard to believe that a weighing millions of times the mass of the sun could be moved at all, let alone kicked out of a galaxy at enormous speed," said Francesca Civano of the Harvard-Smithsonian Center for Astrophysics (CfA), who led the new study. "But these new data support the idea that gravitational waves -- ripples in the fabric of space first predicted by Albert Einstein but never detected directly -- can exert an extremely powerful force."

Although the ejection of a supermassive black hole from a galaxy by recoil because more gravitational waves are being emitted in one direction than another is likely to be rare, it nevertheless could mean that there are many giant black holes roaming undetected out in the vast spaces between galaxies.

"These black holes would be invisible to us," said co-author Laura Blecha, also of CfA, "because they have consumed all of the gas surrounding them after being thrown out of their home galaxy."

Civano and her group have been studying a system known as CID-42, located in the middle of a galaxy about 4 billion light years away. They had previously spotted two distinct, compact sources of in CID-42, using NASA's .

More optical data from the ground-based Magellan and Very Large Telescopes in Chile supplied a spectrum (that is, the distribution of optical light with energy) that suggested the two sources in CID-42 are moving apart at a speed of at least 3 million miles per hour.

Previous Chandra observations detected a bright X-ray source likely caused by super-heated material around one or more supermassive black holes. However, they could not distinguish whether 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 previous data told us that there was something special going on, but we couldn't tell if there were two black holes or just one," said another co-author Martin Elvis, also of CfA. "We needed new X-ray data to separate the sources."

When Chandra's sharp High Resolution Camera was pointed directly at CID-42, the resulting data showed that X-rays were coming only from one of the sources. The team thinks that when two galaxies collided, 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, which gave the newly merged black hole a sufficiently large kick for it to eventually escape from the galaxy. The other optical source is thought to be the bright star cluster that was left behind. This picture is consistent with recent computer simulations of merging black holes, which show that merged black holes can receive powerful kicks from the emission of gravitational waves.

There are two other possible explanations for what is happening in CID-42. One would involve an encounter between three supermassive black holes, resulting in the lightest one being ejected. Another idea is that CID-42 contains two supermassive black holes spiraling toward one another, rather than one moving quickly away.

Both of these alternate explanations would require at least one of the supermassive to be very obscured, since only one bright X-ray source is observed. Thus the Chandra data support the idea of a black hole recoiling because of .

The source is located in the Cosmic Evolution Survey (COSMOS) field, a large, multi-wavelength survey.

These results will appear in the June 10 issue of The Astrophysical Journal.

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3.3 / 5 (7) Jun 04, 2012
There's some of the dark matter explained...
1.2 / 5 (5) Jun 04, 2012
It's possible the other black hole is the remnant of another galaxy consumed. For example the Andromeda galaxy has a 2nd massive black hole near its core observable too. The existence of multiple nuclei seems to be rather rule than an exception at the case of large galaxies: for example our Milky Way core exhibits multiple black holes as well. It corresponds the finding, most of stars in the Universe are actually binary stars. I'd say, the objects in Universe prefer to live in harmonic families in similar way, like the people do.
1.4 / 5 (15) Jun 04, 2012
So is the accretion disk also ejected moving along at 3 Mmph? Doubtful. Why then is it visible? Answer: the supermassive core star is generating matter and energy from within via a dimension outside our detectable universe. Easy as pie. No need to remain confused.

LaViolette has commented extensively on an earlier discovery of a daughter galactic core star being ejected from the parent galaxy. This is simply likely another example.


And for my original explanation for what is happening, for those new readers with, at least, a little willingness to consider alternative cosmogenic models....

1 / 5 (3) Jun 05, 2012
Presumably, they infer the high differential velocity from differential red-shift. And they struggle to explain how this could be possible. However, I would suggest it is more likely that the differential red-shift is more likely due to non-cosmological origins, as LaViolette suggests in this quasar observation inside a parent galaxy.


One of the two core stars is likely more massive than the other, producing a deeper gravity well, which in SubQuantum Kinectics physics, results in a greater red shift. As the light climbs out of the gravity well, it is red-shifted. And as LaViolette points out, there are likely other factors that further contribute to the red shift.

Isn't it time to revisit the various causes of red-shift, rather that attributing it entirely to recessional velocity?

It must be cake, if I can figure it out....

not rated yet Jun 06, 2012
Giant black hole kicked out of home galaxy

What does a SMBH gotta do to get some respect?
1 / 5 (1) Jun 07, 2012
However, I would suggest it is more likely that the differential red-shift is more likely due to non-cosmological origins, ...

As the light climbs out of the gravity well, it is red-shifted.

Isn't it time to revisit the various causes of red-shift, rather that attributing it entirely to recessional velocity?

Gravitational redshift is well known, proven and quantified by the Pound-Rebka Experiment and observed in the spectrum of the Sun. The amount of redshift is tiny compared to these observations.

The cranks can always come up with inventive hand-waving explanations but the numbers give them away.

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