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The nebular emission of star-forming galaxies in a hierarchical universe
Alvaro Orsi, Nelson Padilla, Brent Groves +4
Galaxy surveys targeting emission lines are characterising the evolution of star-forming galaxies, but there is still little theoretical progress in modelling their physical proper…
Mid-Infrared Atomic Fine-Structure Emission Line Spectra of Luminous Infrared Galaxies: Spitzer/IRS Spectra of the GOALS Sample
H. Inami, L. Armus, V. Charmandaris +18
We present the data and our analysis of MIR fine-structure emission lines detected in Spitzer/IRS high-res spectra of 202 local LIRGs observed as part of the GOALS project. We dete…
Theoretical Evolution of Optical Strong Lines across Cosmic Time
Lisa J. Kewley, Michael A. Dopita, Claus Leitherer +5
We use the chemical evolution predictions of cosmological hydrodynamic simulations with our latest theoretical stellar population synthesis, photoionization and shock models to pre…
Andromeda's Dust
B. T. Draine, G. Aniano, Oliver Krause +10
Spitzer Space Telescope and Herschel Space Observatory imaging of M31 is used, with a physical dust model, to construct maps of dust surface density, dust-to-gas ratio, starlight h…
Mapping dust through emission and absorption in nearby galaxies
K. Kreckel, B. Groves, E. Schinnerer +13
Dust has long been identified as a barrier to measuring inherent galaxy properties. However, the link between dust and attenuation is not straightforward and depends on both the am…
On the effect of the Cosmic Microwave Background in high-redshift (sub-)millimeter observations
Elisabete da Cunha, Brent Groves, Fabian Walter +11
Modern (sub-)millimeter interferometers enable the measurement of the cool gas and dust emission of high-redshift galaxies (z>5). However, at these redshifts the cosmic microwave b…