黑洞

中等質量黑洞

zhong ˉ dengˇ zhiˊ liangˋ hei ˉ dongˋ

(Black holes, Intermediate-mass)

Intermediate-mass black holes, Black holes with a mass in the range of 100 to 100 000 (or even 1 000 000) solar masses

Cat: Astronomy (Intermediate-mass black holes) ^Next

>>中等質量黑洞

中, 等, 質, 量, 黑, 洞

超大質量黑洞

chao ˉ daˋ zhiˊ liangˋ hei ˉ dongˋ

(Black Hole, Supermassive)

Supermassive black hole (SMBH, SBH), A black hole possessing as much mass as a million or a billion stars; They reside in the centers of galaxies and are the engines that power active galactic nuclei and quasars

Cat: Astronomy (Supermassive black hole (SMBH, SBH)) ^Next

>>超大質量黑洞

超, 大, 質, 量, 黑, 洞

以黑洞為中心的恆
星系統

yiˇ hei ˉ dongˋ weiˋ zhong ˉ xin ˉ de˙ hengˊ
xing ˉ xiˋ tongˇ

(Star System)

A star system with a black hole at its center

>>以黑洞為中心的恆星系統

以, 黑, 洞, 為, 中, 心, 的, 恆
星, 系, 統

恆星級黑洞

hengˊ xing ˉ jiˊ hei ˉ dongˋ

(A black, Stellar-mass)

Stellar-mass black hole, A black hole (typically between 3 and 10 solar masses) that forms when a massive star explodes and leaves behind a small, heavy core which collapses on itself if it has enough mass

Cat: Astronomy (Stellar-mass black hole) ^Next

>>恆星級黑洞

恆, 星, 級, 黑, 洞

史瓦西黑洞

shiˇ waˇ xi ˉ hei ˉ dongˋ

(A black, Schwarzschild)

Schwarzschild black hole, A black hole with no electric charge and no angular-momentum (which means it is non-rotating) that has an event horizon radius determined solely by its mass; The Schwarzschild metric describes such a black hole and was worked out by Karl Schwarzschild (and independently by Johannes Droste) in 1916

Cat: Astronomy (Schwarzschild black hole) ^Next

>>史瓦西黑洞

史, 瓦, 西, 黑, 洞