However, there is little central concentration of the X-ray emission.
This X-ray emission has since been decaying in a variable manner.
It has an X-ray emission of 8.2 x 10 erg s.
The satellite cannot see anything but a flickering point of X-ray emission.
With a probability of 99.4%, this companion is the source for the X-ray emission from the system.
The energy source for the X-ray emission is gravity.
It may be the source of the X-ray emission from the vicinity.
However, even to this day, the process which gives rise to the X-ray emissions is controversial.
So far, the team has observed there has been a 35 percent in X-ray emission from 2000 to 2008.
The source for this strong X-ray emission is the star's hot corona.
