Blue Supergiant Stars蓝超巨星
Blue supergiant stars are typically characterized by an O-Type spectrum, or a B-type spectrum for those classified as blue-white. 蓝超巨星通常具有O型光谱,或对于被归类为蓝白色的恒星而言为B型光谱。
|
Index Star concepts 索引星概念 | ||
|
Go Back
返回 |
Deneb天琴座α星
Blue-white stars are typically characterized by a B-type spectrum. 蓝白色星通常具有B型光谱。
|
Index Star concepts Blue supergiant stars 索引星概念 蓝超巨星 | ||
|
Go Back
返回 |
Sk-69202, Progenitor of SN 1987ASk-69202,超新星1987A的前身星
It was fortunate that the star which produced Supernova 1987A was a known star, a blue supergiant star which had been catalogued as SK-69202. It presumed to have a mass of about 20 solar masses. 幸运的是,产生超新星1987A的恒星是一颗已知的蓝超巨星,曾被编目为SK-69202。它被假定具有约20个太阳质量。
Blue supergiant stars are typically characterized by an O-Type spectrum. 蓝超巨星通常具有O型光谱。
|
Index Star concepts Blue supergiant stars 索引星概念 蓝超巨星 | ||
|
Go Back
返回 |