对空间飞行器在Be恒星中可观测到的[Fe II]、[Fe III]、[Ni II]和[Ni III]禁止条纹的考虑

J. Swings
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引用次数: 0

摘要

[Fe II], [Fe III], [Ni II]和[Ni III]的最强禁跃迁已经被计算出来,作为准备用空间飞行器对明线星进行光谱观测的初步步骤。几个预测的禁止发射肯定起着重要的作用,特别是在红外区域。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Considérations sur les raies interdites de [Fe II], [Fe III], [Ni II] et [Ni III] observables dans les étoiles Be, par véhicules spatiaux
The strongest forbidden transitions of [Fe II], [Fe III], [Ni II] and [Ni III] have been computed as a preliminary step in the preparation of spectroscopic observations of bright line stars with space vehicles. Several predicted forbidden emissions play certainly an important role, especially in the infrared region.
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