arXivDaily arXiv每日学术速递 周一至周五更新
北美退伍军人节(Veterans Day),12 日无更新
arXiv 2407.16784astro-ph.GA
收藏

渗透银河系CGM的亚太阳Fe/O、logT~7.5气体成分

A Sub-solar Fe/O, logT~7.5 Gas Component Permeating the Milky Way's CGM

Armando Lara-DI, Yair Krongold, Smita Mathur, Sanskriti Das, Anjali Gupta, O. Segura Montero

AI总结:

本研究利用叠加的Chandra光谱和PHASE代码建模,发现银河系CGM中存在温度均匀但柱密度不均的hot气体成分,其非太阳丰度比表明该超位力气体相起源于星系反馈。

摘要:

我们的研究重点是表征银河系(MW)环星系介质(CGM)内的高电离气体,这些气体在2-25 Å的X射线波段产生离子跃迁。利用叠加的Chandra/ACISS MEG和LETG朝向类星体(QSO)视线方向的观测光谱,我们采用自洽的混合电离代码PHASE对数据进行建模。叠加光谱最优地由三个不同的气体相成分描述:warm(logT ~ 5.5)、warmhot(logT ~ 6)和hot(logT ~ 7.5)成分。这些发现证实了MW的CGM中存在hot成分,表明其与warm和warmhot气体相共存。我们发现该hot成分在温度上是均匀的,但在柱密度上是不均匀的。为了与文献中报告的银河系晕的色散测量(DM)一致,hot成分中的气体需要相对于太阳的过丰度。对于hot相,我们估计的DM = 55.1^{+29.9}_{-23.7} pc cm^{-3}。我们得出结论,该相要么在氧、硅和硫中富集,要么其金属丰度超过太阳值的6倍,或者是两者的结合。我们未检测到Fe L壳层吸收线,这意味着O/Fe ≥ 4。在银河系晕的超位力气体成分中发现的非太阳丰度比表明,该相起源于星系反馈。

英文摘要:

Our study focuses on characterizing the highly ionized gas within the Milky Way's (MW) Circumgalactic Medium (CGM) that gives rise to ionic transitions in the X-ray band 2 - 25 Å. Utilizing stacked \Chandra/\ACISS\ \MEG\ and \LETG\ spectra toward QSO sightlines, we employ the self-consistent hybrid ionization code PHASE to model our data. The stacked spectra are optimally described by three distinct gas phase components: a \warm\ (\logT\ $\sim$ 5.5), \warmhot\ (\logT\ $\sim 6$), and \hot\ (\logT\ $\sim$ 7.5) components. These findings confirm the presence of the \hot\ component in the MW's CGM indicating its coexistence with a \warm\ and a \warmhot\ gas phases. We find this \hot\ component to be homogeneous in temperature but inhomogeneous in column density. The gas in the \hot\ component requires over-abundances relative to solar to be consistent with the Dispersion Measure (DM) from the Galactic halo reported in the literature. {For the hot phase we estimated a DM = $55.1^{+29.9}_{-23.7}$ pc cm$^{-3}$}. We conclude that this phase is either enriched in Oxygen, Silicon, and Sulfur, or has metallicity {over 6} times solar value, or a combination of both. We do not detect Fe L-shell absorption lines, implying O/Fe $\geq$ 4. The non-solar abundance ratios found in the super-virial gas component in the Galactic halo suggest that this phase arises from Galactic feedback.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

↑