If the swirling disk of gas is massive enough-one-tenth the mass of its star or more-johns-krull says the gravitational power of the disk can make the disk unstable.
如果漩磁盘的气体足够大—它的恒星的十分之一或更多—磁盘的重力能够是磁盘动荡，约翰斯说到。
Astronomers have found a disk of dust around a huge, massive star in its early stages of growth, indicating that stars big and small form by the same mechanism.
天文学家发现一个碟状的尘埃围绕着一个巨型星体，该星体正在它的成长阶段，说明星体无论大小，形成的机制是一样的。
They "clearly show that at least some massive stars grow by accreting material from a circumstellar disk of gas and dust, just like our sun did roughly 4.5 billion years ago."
它们‘清楚地显示了至少一些巨型恒星由环绕的碟状气体和尘埃凝聚而成，就如我们的太阳在45亿年前一样。’
Van den Bosch is particularly intrigued by the formation of disk galaxies and of massive black holes in galactic centers.
范登柏希特别著迷于盘形星系与星系中心超大质量黑洞的形成过程。
As the accretion disk feeds more mass into itself, the embryo star contracts, growing ever denser and more massive.
随著吸积盘获得越来越多的物质，胚胎恒星就不断收缩，密度和质量都变得越来越大。
Cataclysmic variables involve gas falling from a large star onto an accretion disk surrounding a massive but compact White Dwarf star.
激变星涵盖了巨星上气体物质掉入环绕著其巨大且紧实的白矮星，而产生围绕白矮星的吸积盘。
Cataclysmic variables involve gas falling from a large star onto an accretion disk surrounding a massive but compact White Dwarf star.
激变星涵盖了巨星上气体物质掉入环绕著其巨大且紧实的白矮星，而产生围绕白矮星的吸积盘。
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