Astronomers have long predicted the presence of
such black holes at the center of the galaxy, which they said could number in the thousands.
Not exact matches
The study appears to vindicate predictions from theorists
such as Mark Morris, an astrophysicist
at the University of California, Los Angeles, who in 1993 penned a key paper predicting tens of thousands of stellar - mass
black holes would form a disk around the galactic
center.
The objects causing these low - frequency ripples —
such as orbiting supermassive
black holes at the
centers of distant galaxies — would be different from the higher frequency ripples, emitted by collisions of much smaller
black holes, that have so far been detected on Earth.
These rapidly spinning neutron stars flash regular radio pulses, and in an upcoming issue of The Astrophysical Journal astronomers say that the timing of
such pulses could provide a new understanding of the 4 million solar mass
black hole at the
center of the Milky Way.
The current model of active galaxies
such as M87 posits that each one harbors
at its
center a
black hole many millions or even billions of times more massive than our own sun, all packed into a space about the size of our solar system.
Previously, astronomers have used x-ray telescopes to observe strong winds very near the massive
black holes at galactic
centers (artist's concept, inset) and infrared wavelengths to detect the vast outflows of cool gas (bluish haze in artist's concept, main image) from
such galaxies as a whole, but they've never done so in the same galaxy.
Resembling spotlights
at a Hollywood movie premier,
such beams are probably generated as matter plunges into a supermassive
black hole at the
center of the galaxy.
The nearly 100 percent polarization of the radio bursts is unusual, and has only been seen in radio emissions from the extreme magnetic environments around massive
black holes,
such as those
at the
centers of galaxies.
Such «supercritical accretion» is thought to be a possible mechanism in the formation of supermassive
black holes at galactic
centers in very short time periods (which are observed very early in cosmic time).
This may help solve
such mysteries as how gas clouds are triggered to form new stars and when the massive
black hole at the
center of every mature galaxy forms.
But Kulkarni counters that
such massive objects should sink even closer to the
center and says the lack of x-rays means they aren't
black holes at all.
Using NASA's super-sensitive Chandra X-ray space telescope, a team of astronomers led by Q. Daniel Wang
at the University of Massachusetts Amherst has solved a long - standing mystery about why most super massive
black holes (SMBH)
at the
centers of galaxies have
such a low accretion rate — that is, they swallow very little of the cosmic gases available and instead act as if they are on a severe diet.
They may have exotic structures
such as supermassive
black holes at their
centers.
On the other hand, if it were a very massive object,
such as a
black hole, it would appear to be
at rest in the Galaxy's
center.