The Thick Accretion Disk Model and Self - gravitating Accretion Disk Model of QSOs.

类星体的厚吸积盘与自引力吸积盘模型.

An accretion disk with vertical structure is studied by using a new anomalous viscosity.

利用一种全新的反常粘滞,主要研究了具有垂向结构的吸积盘.

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

为我们相信吸积盘本身是被磁化的，圆盘的旋转可将磁力线扭曲成螺旋线圈状。

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

为我们相信吸积盘本身是被磁化的，圆盘的旋转可将磁力线扭曲成螺旋线圈状。

Active galaxies give off bright radiation from their cores, where gas heats up as it is compressed into a swirling accretion disk encircling the black hole.

活动星系从它们的核部发出明亮的光芒，在那里，气体被加热并压缩成一个漩涡状的圆盘，漩涡的中心便是黑洞。