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The FERRUM project: experimentally determined metastable lifetimes and transition probabilities for forbidden [Ti II] lines observed in eta Carinae

机译:FERRUm项目:实验确定在eta Carinae中观察到的禁用[Ti II]系的亚稳生命期和转移概率

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摘要

In the spectrum of an emission-line region ejected from the massive star Eta Carinae, called the strontium filament (SrF), forbidden lines from many elements, in particular [Sr II] and [Ti II], are observed. These lines are strong in this specific region and valuable for plasma diagnostics. Forbidden lines are not easily produced in laboratory light sources and the atomic parameters for these lines can thus not be measured in a straightforward way. We use a combination of laboratory and astrophysical measurements to determine transition probabilities for the [Ti II] lines. Lifetimes for metastable levels in Ti II are measured using a laser probing technique on a stored ion beam at CRYRING, MSL, Stockholm. Branching fractions from some of these levels are derived from Hubble Space Telescope/STIS spectra of the SrF. The astrophysical branching fractions are combined with the experimental lifetimes to determine absolute transition probabilities. We report lifetimes for the Ti II levels b(4)P(3/2), b(2)P(1/2), c(2)D(3/2) and c(2)D(5/2), in the range 0.29-17 s, and transition probabilities for eight parity-forbidden lines from the levels c(2)D(3/2) and c(2)D(5/2), along with uncertainty estimates.
机译:在从大型恒星Eta Carinae发出的发射线区域的光谱中,观察到被称为锶丝(SrF)的禁线,其中包括许多元素,特别是[Sr II]和[Ti II]。这些线在该特定区域很强,对于血浆诊断很有价值。在实验室光源中不容易产生禁线,因此无法以直接的方式测量这些线的原子参数。我们使用实验室和天体测量的组合来确定[Ti II]谱线的跃迁概率。使用激光探测技术,在斯德哥尔摩CMS的CRYRING上,使用激光探测技术测量Ti II中亚稳态水平的寿命。这些水平中某些水平的分支分数来自SrF的哈勃太空望远镜/ STIS光谱。天体分支分支分数与实验寿命相结合,以确定绝对跃迁概率。我们报告了Ti II级b(4)P(3/2),b(2)P(1/2),c(2)D(3/2)和c(2)D(5/2)的寿命),范围为0.29-17 s,以及从水平c(2)D(3/2)和c(2)D(5/2)开始的八条奇偶禁止线的过渡概率以及不确定性估计。

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