Seeing Through the Dust: The Detection of HI and the Exploration of the ISM in Galaxies

By A. Taylor, T. Landecker, A. Willis. 2002

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The GALAH survey and Gaia DR2: dissecting the stellar disc’s phase space by age, action, chemistry, and location (2018, background): “As far as we can tell, this has not been found locally in recent surveys (Kalberla & Kerp 2009), but there may be evidence for such behaviour at other radii (e.g. Lockman 2002).”
Global properties of the H I distribution in the outer Milky Way - Planar and extra-planar gas (2008, unknown): “Supershells and chimneys may reach z distances of several kpc but appear not to be able to shape a significant fraction of the halo (McClure-Griffiths et al. 2006). As a halo model therefore we have chosen the simple case of a quasi-static system that can be approximated numerically by a hydrostatic”
The mass distribution and gravitational potential of the Milky Way (2016, background): “3 For example,Lockman(2002) note that the surface density plot from Dame(1993), which has been reproduced without comment in standard texts, includes values that have been arbitrarily scaled bya factor of 2.”
The Southern Galactic Plane Survey: H I Observations and Analysis (2005, background): “The IGPS consists of three individual surveys: the Canadian Galactic Plane Survey (CGPS; Taylor et al. 2003), the VLAGalactic Plane Survey (VGPS; Taylor et al. 2002), and the Southern Galactic Plane Survey (SGPS, described here).”