Caught in the Act: A Metal-Rich High-Velocity Cloud in the Inner Galaxy
Frances H. Cashman, Andrew J. Fox, Bart P. Wakker, Trisha Ashley,, Derck Massa, Edward B. Jenkins, Dhanesh Krishnarao, Felix J. Lockman, Robert, A. Benjamin, Rongmon Bordoloi, and Tae-Sun Kim

TL;DR
This study characterizes a metal-rich high-velocity cloud in the inner Galaxy, revealing its physical conditions, chemical composition, and likely origin as part of a Galactic wind outflow.
Contribution
It provides detailed measurements of the cloud's metallicity, ionization states, and dust content, offering new insights into the nature of Galactic outflows and high-velocity clouds.
Findings
High metallicity of [O/H] = +0.36 in the HVC.
Multi-phase hot plasma with temperatures around 10^4.9 K and 10^5.4 K.
Evidence supporting a Galactic wind origin for the cloud.
Abstract
We characterize the chemical and physical conditions in an outflowing high-velocity cloud in the inner Galaxy. We report a super-solar metallicity of [O/H] = for the high-velocity cloud at = 125.6 km s toward the star HD 156359 ( = 328.7, = 14.5, = 9 kpc, = 2.3 kpc). Using archival observations from FUSE, HST STIS, and ESO FEROS we measure high-velocity absorption in H I, O I, C II, N II, Si II, Ca II, Si III, Fe III, C IV, Si IV, N V, and O VI. We measure a low H I column density of log (H I) = in the HVC from multiple unsaturated H I Lyman series lines in the FUSE data. We determine a low dust depletion level in the HVC from the relative strength of silicon, iron, and calcium absorption relative to oxygen, with [Si/O]=, [Fe/O]=, and [Ca/O] =.…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Stellar, planetary, and galactic studies · Bee Products Chemical Analysis
