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arXiv 1105.4757astro-ph.SR
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O2-3 */ WN5-7星的光谱分类

Spectral Classification of O2-3.5If*/WN5-7 stars

Paul Crowther, Nolan Walborn

摘要:

在最近对O型和WN型恒星光谱分类进行修订之后,提出了一个更新的O 2 -3.5If*/WN 5 -7型过渡恒星的分类方案。我们提出用H β的形态学来追踪风密度的增加,可以区分O2 - 3.5If*、O2-3.5If*/WN 5 -7和WN 5 -7星:O2-3.5If* 星的纯吸收,除了Walborn等的常规诊断;天鹅座P O2-3.5If*/WN 5 -7星;纯粹在发射WN星除了通常的诊断从史密斯等人。我们还讨论了近似的标准来区分这些亚型从近红外光谱。定性地讨论了这类恒星的物理和风的性质及其演化意义。我们认为,大多数O2-3.5If*/WN 5 -7恒星是年轻的,非常大质量的氢燃烧恒星,真正的中间O2-3.5If* 和WN 5 -7亚型,虽然少数显然是核心氦燃烧恒星向蓝向经典WN序列。最后,我们重新评估分类的恒星表现出较低的电离光谱特征,加上β发射。

英文摘要:

An updated classification scheme for transition O2-3.5If*/WN5-7 stars is presented, following recent revisions to the spectral classifications for O and WN stars. We propose that O2-3.5If*, O2-3.5If*/WN5-7 and WN5-7 stars may be discriminated using the morphology of Hbeta to trace increasing wind density as follows: purely in absorption for O2-3.5If* stars in addition to the usual diagnostics from Walborn et al.; P Cygni for O2-3.5If*/WN5-7 stars; purely in emission for WN stars in addition to the usual diagnostics from Smith et al. We also discuss approximate criteria to discriminate between these subtypes from near-IR spectroscopy. The physical and wind properties of such stars are qualitatively discussed together with their evolutionary significance. We suggest that the majority of O2-3.5If*/WN5-7 stars are young, very massive hydrogen-burning stars, genuinely intermediate between O2-3.5If* and WN5-7 subtypes, although a minority are apparently core helium-burning stars evolving blueward towards the classical WN sequence. Finally, we reassess classifications for stars exhibiting lower ionization spectral features plus Hbeta emission.

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