white dwarf star

基本解釋

This leads the researchers to suspect that a white dwarf star strayed too close to the intermediate-mass black hole and was ripped apart by tidal forces.
這導(dǎo)致研究人員懷疑一個(gè)迷途的白矮星離某個(gè)中等質(zhì)量黑洞太接近了，并受其潮汐引力的撕扯。
In a later stage of the sun's death throes, when it contracts into a compact white dwarf star, part of this rocky material could rain down into the white dwarf's hot atmosphere.
在垂死掙扎的后期，太陽會(huì)收縮成為高密度的白矮星，這時(shí)部分巖石物質(zhì)可能會(huì)降落到白矮星熾熱的大氣中。
xiaolan.0217.blog.163.com
The primary target is a white dwarf star known as GD358 in the constellation Hercules.
第一顆目標(biāo)恒星是武仙星群中一顆稱為GD358的白矮星。

These new models of failed supernovae demonstrate how both normal brightness and extremely dim supernovae are generated from the same basic picture of a nuclear-burning white dwarf star, he added.
FORBES: When A Supernova ... Fizzles
Standard Type Ia supernovae are binary systems in which a white dwarf star draws so much matter from its companion (often a red giant) that it undergoes a kind of energy overload and detonates.
FORBES: When A Supernova ... Fizzles