4 papers
Theoretical expectations for magnetic field measurements in molecular cloud cores
F. Heitsch, P. S. Li
The currently most viable methods to estimate magnetic field strengths in molecular cloud cores are Zeeman measurements and the Chandrasekhar-Fermi (CF) method. The CF-method estim…
Stellar Populations and Galaxy Morphology at High Redshift
Andrew Bunker, Hyron Spinrad, Daniel Stern +4
In this article we investigate the morphology and stellar populations of high-redshift galaxies through multi-waveband HST imaging and ground-based spatially-resolved spectroscopy.…
Near-Infrared Emission Line Searches for High-Redshift Galaxies
Andrew Bunker
In this article I review recent developments in near-infrared emission line searches for star-forming galaxies at high redshift. Using the J-, H- & K-bands we can potentially chart…
Models and Observations of the Chemistry near Young Stellar Objects
Ewine F. van Dishoeck, Michiel R. Hogerheijde
The study of the chemical evolution of gas and dust from pre-stellar dense cores to circumstellar disks around young stars forms an essential part of understanding star- and planet…