Joss Bland-Hawthorn

TL;DR: In this paper, the physical conditions, elemental abundances, and kinematics of the high-velocity clouds (HVCs) along the sight lines toward active galaxies HE 0226-4110 and PG 0953+414 using Hubble Space Telescope Space Telescope Imaging Spectrograph and Far Ultraviolet Spectroscopic Explorer data.

TL;DR: In this article, the authors decompose the galaxy into three major components, a bulge, a Miyamoto-Nagai disk, and a Navarro-Frenk-White dark matter halo, and then model the kinematic data of the halo blue horizontal branch and K-giant stars from the Sloan Extension for Galactic Understanding and Exploration.

TL;DR: The Survey for Ionization in Neutral Gas Galaxies (SINGG) as mentioned in this paper is a survey of star formation in H I selected galaxies, which consists of H alpha and R-band imaging of a sample of 468 galaxies selected from the H I Parkes All Sky Survey (HIPASS).

TL;DR: In this article, the two-point correlation functions in redshift space were calculated for galaxies of different spectral types in the 2dF Galaxy Redshift Survey, and the correlation function slopes were respectively 1.93 and 1.50.

TL;DR: In this paper, a series of three-dimensional simulations of a starburst-driven wind in an inhomogeneous interstellar medium is performed, and the authors find that soft X-ray emission arises from gas that has been massloaded from clouds in the disk, as well as from bow shocks upstream of clouds, driven into the flow by the ram pressure of the wind, and interaction between these shocks.