General relativistic spectra of accretion discs around rapidly
... result, the plotted spectra for these two cases lie almost on top of each other. However, for i ¼ 08 the flux corresponding to the massshed configuration is slightly higher than that for V ¼ 0, while the case is opposite at higher inclinations. This is a result of the inclination dependence of the ð ...
... result, the plotted spectra for these two cases lie almost on top of each other. However, for i ¼ 08 the flux corresponding to the massshed configuration is slightly higher than that for V ¼ 0, while the case is opposite at higher inclinations. This is a result of the inclination dependence of the ð ...
Neutron Stars, Pulsars, Magnetars – the “corpses” of medium
... If the pulsar can steal enough gas from the red giant, it will grow smaller (more dense) and accelerate its spin. A pulsar can speed up from a few seconds between pulses to just milliseconds between ...
... If the pulsar can steal enough gas from the red giant, it will grow smaller (more dense) and accelerate its spin. A pulsar can speed up from a few seconds between pulses to just milliseconds between ...
How can we explain magnetism?
... Magnetic Force •Created when a moving charge passes through a magnetic field •Reason: Charge has a magnetic field and it interacts with another magnetic field •Greatest force is when the charge passes perpendicular to the field ...
... Magnetic Force •Created when a moving charge passes through a magnetic field •Reason: Charge has a magnetic field and it interacts with another magnetic field •Greatest force is when the charge passes perpendicular to the field ...
