At the American Astronomical Society (AAS) meeting now under way in Washington, DC, several teams of astronomers have announced new advances in understanding the giant black holes that inhabit the centers of nearly all large galaxies. And one group has announced the first evidence of a star being ripped apart by a medium-sized black hole, a variety that astronomers have not been sure exists.
In recent years, astronomers have found that every time they search the heart of a large galaxy that has a central bulge of old stars, they find a black hole with about a million to several billion times the mass of the Sun. But what happens when two large galaxies collide and merge, a scenario that has played out countless times in the universe’s history? Numerous studies suggest that the two black holes should go into orbit around each other and eventually spiral together and merge but not for a long time. If this picture is correct, astronomers ought to find many galaxies with two supermassive holes.
The problem is, astronomers have searched nearby galaxies for double black holes for many years and have only found a handful of convincing candidates. But at a press conference Monday at the AAS, a group led by Julia Comerford of the University of California at Berkeley announced 33 galaxies that have two. “We have discovered 33 pairs of these waltzing supermassive black holes,” she said. “This result is significant because it shows us that they are much more common than previously known from observations.”
All but one of the pairs come from an analysis of several thousand very distant galaxies observed in the DEEP2 Galaxy Redshift Survey (the other comes from the COSMOS galaxy survey). Many of these have supermassive holes that are actively swallowing gas, making their surroundings shine bright. Comerford and her colleagues identified 33 paired cases, in which one active nucleus is moving at high speed (a few hundred kilometers per second, or roughly 500,000 miles per hour) with respect to the host galaxy and its own nucleus.
The black holes in each pair are typically a few thousand light-years apart, meaning they are not yet close enough to each other to go into a tight orbit. For this reason, Comerford describes them as “dual black holes,” and not true binary black holes.
But as the interloper gravitationally stirs up the stars and gas that it passes, it loses momentum. So it should eventually sink to the center to form a true binary with the galaxy's native hole. Their inspiral and eventual merger should be a long, drawn-out process that will take hundreds of millions or billions of years.
Another group, led by Francesca Civano of the Harvard-Smithsonian Center for Astrophysics, studied X-ray and optical spectra of one of those 33 galaxies and found evidence that a black hole that already resulted from a merger 1 to 10 million years ago is shooting away from the galaxy’s center at the incredible speed of at least 1,300 km per second (3 million miles per hour). The simplest explanation is that it was born from the merger of two unequal black holes. Computer simulations indicate that gravitational radiation emitted asymmetrically as such holes merge can give the end product a huge kick, in some cases enough to eject it clear out of its galaxy. Civano says the measured radial velocity of this fast-moving hole is consistent with such a kick, but that further observations are needed to determine if this interpretation is correct.
A third group, led by Ruth Daly of Penn State University, studied 55 supermassive black holes that are producing powerful high-speed particle jets. Using a new method that she published last year, Daly estimated each hole’s spin from the jet’s power. She found a wide range of black-hole spins among her 55 objects. The most distant of them, up to 10 billion light-years away and seen when the universe was young, spin at the maximum speed theoretically possible. But closer black holes, some just a few tens of millions of light-years away in essentially the present-day universe, spin at only about 10% to 80% of their theoretical maximum speed.
A fourth group looked for unusual activity around suspected "intermediate- mass" black holes, those with perhaps a few thousand times the mass of the Sun. Astronomers have sought this variety for decades and found several very strong candidates. But conclusive proof does not yet exist, and the field remains rife with controversy. Some of the best candidates have been found in the centers of globular clusters, collections of several hundred thousand ancient stars.
The team, led by Jimmy Irwin of the University of Alabama, studied a globular cluster in the fringes of elliptical galaxy NGC 1399, located about 65 million light-years away in Fornax. Unlike most globulars, this one shows strong X-ray emission. The strength and other characteristics of the X-ray blaze ("ULX" in the image at right) suggest that the hole has an intermediate mass much greater than the stellar-mass black holes.
Visible-light spectra show large amounts of the relatively heavy elements oxygen and nitrogen in its hot stuff, but no hydrogen. Heavy elements aren't found in gaseous form in globular clusters but they would be expected if an old white-dwarf star were torn to gaseous shreds by passing very close to a black hole.
Although other explanations remain very much in play, Irwin said this is the first evidence that an intermediate-mass black hole ripped apart a star. “If our assumptions are true,” he added, “we found the first stellar disruption event in a globular cluster, and that intermediate-mass black holes exist in the universe.”
As with most results presented at conferences, these results have yet to be fully vetted by the astronomical community and have not been independently confirmed.