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Comprehensive comparison of models for spectral energy distributions from 0.1 micron to 1 mm of nearby star-forming galaxies
L. K. Hunt, I. De Looze, M. Boquien +26
We have fit the far-ultraviolet (FUV) to sub-millimeter (850 micron) spectral energy distributions (SEDs) of the 61 galaxies from the "Key Insights on Nearby Galaxies: A Far-Infrar…
Absorption by Spinning Dust: a Contaminant for High-Redshift 21 cm Observations
B. T. Draine, Jordi Miralda-Escudé
Spinning dust grains in front of the bright Galactic synchrotron background can produce a weak absorption signal that could affect measurements of high redshift 21 cm absorption. A…
Electron Energy Distributions in HII Regions and Planetary Nebulae: kappa-Distributions Do Not Apply
B. T. Draine, C. D. Kreisch
Some authors have proposed that electron energy distributions in H II regions and planetary nebulae may be significantly nonthermal, and kappa-distributions have been suggested as…
The State-of-Play of Anomalous Microwave Emission (AME) Research
Clive Dickinson, Y. Ali-Haïmoud, A. Barr +30
Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range -60 GHz. AME was first detected in 1996 and recogni…
After The Fall: The Dust and Gas in E+A Post-Starburst Galaxies
A. Smercina, J. D. T. Smith, D. A. Dale +11
The traditional picture of post-starburst galaxies as dust- and gas-poor merger remnants, rapidly transitioning to quiescence, has been recently challenged. Unexpected detections o…