星壳 meaning in Chinese
star crust
Examples
- Both changes make the star tend to shrink, which induces stresses in the crust .
这两种变化都会使星体收缩，因而在星壳中产生应力。 - We believe there is a solid crust of heavy nuclei , which is about 1 km thick . below it is a layer of neutrons in liquid state . there may be a solid core , but we are not sure
我们相信中子星有一层约一公里厚由重原子核组成的外星壳，之下是一层呈液态的中子流质，最后可能是一个固体核心。 - The infrared carbon stars , whose infrared spectra are mainly due to the dust emission in the circumstellar envelope , are usually believed to be surrounded by the carbon rich envelope characterized by the sic emission feature at 11 . 3um
红外碳星常被认为有很厚的富碳拱星壳层，它的红外光谱主要表现为源于拱星壳层的尘埃发射，这个尘埃发射主要以11 . 3 m的sic发射为标记。 - Visual carbon stars whose mid - infrared spectra are mainly dominated by photospheric continuum and show large excesses at 60um , represent a transition phase which follows an interruption of mass loss from the oxygen - rich phase and begins a new phase of the mass loss of carbon - rich material . excesses at 60um in these stars are the emission from the residual of oxygen - rich material
光学碳星的中红外能量主要来自光球，在60 m处存在超量发射，人们认为其演化阶段处在抛射富氧物质终止和新的富碳拱星壳层形成之间，其60 m超量发射就是富氧物质的残余效应。