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A self-consistent model of Galactic stellar and dust infrared emission and the abundance of polycyclic aromatic hydrocarbons
Thomas P. Robitaille, Ed Churchwell, Robert A. Benjamin +4
We present a self-consistent three-dimensional Monte-Carlo radiative transfer model of the stellar and dust emission in the Milky-Way, and have computed synthetic observations of t…
Distances to Dark Clouds: Comparing Extinction Distances to Maser Parallax Distances
Jonathan B. Foster, Joseph J. Stead, Robert A. Benjamin +2
We test two different methods of using near-infrared extinction to estimate distances to dark clouds in the first quadrant of the Galaxy using large near infrared (2MASS and UKIDSS…
Characterizing Transition Temperature Gas in the Galactic Corona
Bart P. Wakker, Blair D. Savage, Andrew J. Fox +1
We present a study of the properties of the transition temperature (T~10^5 K) gas in the Milky Way corona, based on measurements of OVI, NV, CIV, SiIV and FeIII absorption lines se…
Vertical structure of a supernova-driven turbulent magnetized ISM
Alex S. Hill, M. Ryan Joung, Mordecai-Mark Mac Low +4
Stellar feedback drives the circulation of matter from the disk to the halo of galaxies. We perform three-dimensional magnetohydrodynamic simulations of a vertical column of the in…