2023ApJ...944...65C -
Astrophys. J., 944, 65 (2023/February-2)
Caught in the Act: A Metal-rich High-velocity Cloud in the Inner Galaxy.
CASHMAN F.H., FOX A.J., WAKKER B.P., ASHLEY T., MASSA D., JENKINS E.B., KRISHNARAO D., BENJAMIN R.A., BORDOLOI R. and KIM T.-S.
Abstract (from CDS):
We characterize the chemical and physical conditions in an outflowing high-velocity cloud (HVC) in the inner Galaxy. We report a supersolar metallicity of [O/H] = +0.36 ± 0.12 for the HVC at vLSR = 125.6 km s–1 toward the star HD 156359 (l = 328.°7, b = -14.°5, d = 9 kpc, z = -2.3 kpc). Using archival observations from the Far-Ultraviolet Spectroscopic Explorer (FUSE), the Hubble Space Telescope Imaging Spectrograph, and the European Southern Observatory Fiber-fed Extended Range Optical Spectrograph 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 N(H I) = 15.54 ± 0.05 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] = -0.33 ± 0.14, [Fe/O] = -0.30 ± 0.20, and [Ca/O] = -0.56 ± 0.16. Analysis of the high-ion absorption using collisional ionization models indicates that the hot plasma is multiphase, with the C IV and Si IV tracing 104.9 K gas and N V and O VI tracing 105.4 K gas. The cloud's metallicity, dust content, kinematics, and close proximity to the disk are all consistent with a Galactic wind origin. As the HD 156359 line of sight probes the inner Galaxy, the HVC appears to be a young cloud caught in the act of being entrained in a multiphase Galactic outflow and driven out into the halo.
Abstract Copyright:
© 2023. The Author(s). Published by the American Astronomical Society.
Journal keyword(s):
Galactic center - Ultraviolet astronomy - High-velocity clouds - Chemical abundances - Galactic winds
Simbad objects:
11
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