accretion disk造句怎么写

) Because the accretion disk itself is believed to be magnetized, the rotation of the disk can twist the magnetic field lines into a helix.

( Dwarf novae, explosions of light from the accretion disk around a white dwarf in a binary system, are examples of this phenomenon.

They go around in the plane of the blackboard, say, and so this matter cannot fall radially in but it will fall in and spiral in and forms what we call an accretion disk around the neutron star.

The effect of dissipation on magnetic instability of accretion disks

X-ray observations of iron in the accretion disks may actually be showing the effects of such a massive black hole as well.

The single black hole-accretion disk precession model or disk-driven precession model is discussed carefully;

Binary star systems containing a pulsar and an accretion disk occur beginning at about 14:30.

Later simulations show that even a companion with an orbit as wide as Neptune's could scoop up an accretion disk.

In the same way, ultraviolet photons from accretion disks around white dwarfs and in active galactic nuclei or quasars may also accelerate winds from the disk.

The most conspicuous effects are believed to come from matter falling into a black hole, which( like water flowing into a drain) is predicted to collect into an extremely hot and fast-spinning accretion disk around the object before being swallowed by it.

The different kinds of think accretion disk models, the accretion disk model for ultraviolet excess and the self-gravitating accretion disk model in QSOs axe briefly reviewed.

As the accretion disk feeds more mass into itself, the embryo star contracts, growing ever denser and more massive.

In some cases, the outflows probably wield a controlling influence on the accretion disk, because they carry not only mass and energy outward but perhaps significant amounts of angular momentum as well.

This formation, called an accretion disk, may be very important in some stellar birth sequences.

The energy release can make accretion disks formidable power sources.

The conclusion is: the short term variability behavior provides a strong support to the thick accretion disk model of AGN.