The clusters are tight knots of hundreds of thousands to millions of stars that orbit
around galactic centers like moths around a streetlamp.
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.
As our solar system slowly orbits
around the galactic center, the sun's ultraviolet radiation carves out an egg - shaped region of ionized hydrogen atoms surrounded by neutral hydrogen gas.
Portegies Zwart says the best place to look is in the plane of the galaxy, in the constellations of Vela and Cygnus, along the sun's trajectory
around the galactic center.
Among other sources of such radiation, scientists have proposed that interactions between bits of dark matter (which make up a large fraction of the universe's mass but haven't yet been directly detected) in a halo
around the galactic center may be creating the surplus gamma rays.
Stars richer in elements heavier than hydrogen and helium have less disordered motions, but are orbiting
around the galactic center faster than older stars that are deficient in heavier elements.
«People have been trying to find a pulsar
around the galactic center for decades,» Falcke notes.
Hooper and his colleagues conclude that annihilations of dark matter particles with a mass between 31 and 40 GeV provide a remarkable fit for the excess based on its gamma - ray spectrum, its symmetry
around the galactic center, and its overall brightness.
In some simulations, the stars spread along a full orbit
around the galactic center.
Although the cluster dissolved over the past 4.6 billion years with the dispersal of the Sun's sibling stars into the surrounding the Milky Way, the stars should have remained on a similar orbit
around the galactic center.
Not exact matches
Our black hole's violent meeting with G2 began last year, and as it continues, it should give astronomers a chance to peer inside the
galactic center — the neighborhood
around the black hole — rather than just simulate the swirling disc of gas and dust surrounding it.
«I had heard there was this trouble understanding the so - called
galactic rotation curves, which describe the way stars rotate
around the
centers of galaxies,» he says.
The comparison clearly showed that the observed rotation can not be explained unless large amounts of dark matter exist
around us, and between us and the
galactic center.
«Roughly speaking, our galaxy looks like a pizza pie with an orange in the
center — that's the
galactic bulge — and then there is a very tenuous halo
around the pie,» he explains.
Years of infrared observations have shown a handful of stars at our
galactic center whipping
around an invisible object with a strong gravitational tug.
In addition, these stars are not orbiting the
galactic center inside the Milky Way's spiral arms like the Sun, but they originate from the spherical
Galactic halo that surrounds the Milky Way's main disk, while briefly intersecting it in their long, elliptical orbits
around the
center.
However, the stars will be thrown into different orbits
around the new
galactic center.
Another idea floating
around is that FRBs are emitted by active
galactic nuclei, or AGNs — superluminous regions at the
centers of some galaxies.
Not only do the types of stars differ in many ways from what we can see in our serene nighttime sky from Earth, but the stars at the
galactic center are also not behaving like the stars
around us.
This means stars orbiting
around a galaxy should feel less gravitational pull — and orbit more slowly — the farther they are from the
galactic center.