Circumgalactic Enrichment in Local Dwarf Galaxies as Probed by Star-Formation Driven Outflows

Michael Romano
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Abstract

Galactic feedback driven by massive stars and active galactic nuclei plays a fundamen-tal role in regulating galaxy formation and evolution. In particular, intense starburst episodes can generate strong outflows able to suppress star formation by expelling large amount of dust and metals out of the galaxies, possibly enriching their circum (or even inter) galactic media. Local dwarf galaxies are particularly sensitive to feedback processes and offer a unique opportunity to study these phenomena in great details. We search for outflow signatures in a sample of ∼ 30 lo-cal dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to detect atomic outflows in the broad wings of observed [CII] 158 µm line profiles. We find that atomic outflows in these galaxies have typical mass-loading factors consistent with unity and velocities high enough to bring gas and dust outward. Our results can be used as input for chemical models, posing new constraints on the processes of dust growth and destruction in the interstellar medium of galaxies.
恒星形成驱动外流探测到的本地矮星系的环银河富集现象
由大质量恒星和活动星系核驱动的星系反馈在调节星系的形成和演化中起着重要的作用。特别是,强烈的星暴事件可以产生强烈的流出物,通过将大量的尘埃和金属排出星系,可能丰富它们的环(甚至是星系间)介质,从而抑制恒星的形成。局部矮星系对反馈过程特别敏感,为详细研究这些现象提供了独特的机会。我们从矮星系调查中提取的¼30低卡矮星系样本中寻找流出信号。我们利用赫歇尔/PACS档案数据来探测观测到的[CII] 158 µm谱线宽翼中的原子流出。我们发现这些星系中的原子外流具有典型的质量加载因子,与单位一致,并且速度足够高,可以向外携带气体和尘埃。我们的结果可以作为化学模型的输入,对星系星际介质中尘埃生长和破坏的过程提出新的限制。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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