A High-Metallicity High Velocity Cloud along the MRK 421 Sight Line: A Tracer of Complex M?
Audio, Transactions of the IRE Professional Group on (2011)
We present a new measurement, 0.85-3.5 Z_solar, of the metallicity of high velocity cloud (HVC) Complex M by analyzing ultraviolet spectroscopic observations of the blazar Mrk 421 taken with the Cosmic Origins Spectrograph on the Hubble Space Telescope and the Far Ultraviolet Spectroscopic Explorer. Although an HVC at V_LSR = -131 km/s is not visible in 21 cm emission (logN_HI<3.5 kpc, above the Galactic plane suggest that Complex M is condensed returning gas from a Galactic fountain.
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