4,403 research outputs found
What shapes the far-infrared spectral energy distributions of galaxies?
To explore the connection between the global physical properties of galaxies
and their far-infrared (FIR) spectral energy distributions (SEDs), we study the
variation in the FIR SEDs of a set of hydrodynamically simulated galaxies that
are generated by performing dust radiative transfer in post-processing. Our
sample includes both isolated and merging systems at various stages of the
merging process and covers infrared (IR) luminosities and dust masses that are
representative of both low- and high-redshift galaxies. We study the FIR SEDs
using principle component analysis (PCA) and find that 97\% of the variance in
the sample can be explained by two principle components (PCs). The first PC
characterizes the wavelength of the peak of the FIR SED, and the second encodes
the breadth of the SED. We find that the coefficients of both PCs can be
predicted well using a double power law in terms of the IR luminosity and dust
mass, which suggests that these two physical properties are the primary
determinants of galaxies' FIR SED shapes. Incorporating galaxy sizes does not
significantly improve our ability to predict the FIR SEDs. Our results suggest
that the observed redshift evolution in the effective dust temperature at fixed
IR luminosity is not driven by geometry: the SEDs of ultraluminous
IR galaxies (ULIRGs) are cooler than those of local ULIRGs not because the
high-redshift galaxies are more extended but rather because they have higher
dust masses at fixed IR luminosity. Finally, based on our simulations, we
introduce a two-parameter set of SED templates that depend on both IR
luminosity and dust mass.Comment: Submitted to ApJ, comments welcom
Virtual Life Sentences: An Exploratory Study
Virtual life sentences are sentences with a term of years that exceed an individual’s natural life expectancy. This exploratory study is one of the first to collect data that establish the existence, prevalence, and scope of virtual life sentences in state prisons in the United States. Initial data reveal that more than 31,000 people in 26 states are serving virtual life sentences for violent and nonviolent offenses, and suggest racial disparities in the distribution of these sentences. This study also presents potential policy implications and suggestions for future research
The Internal Ultraviolet-to-Optical Color Dispersion: Quantifying the Morphological K-Correction
We present a quantitative measure of the internal color dispersion within
galaxies, which quantifies differences in morphology as a function of
wavelength. We apply this statistic to a local galaxy sample with archival
images at 1500 and 2500 Angstroms from the Ultraviolet Imaging Telescope, and
ground-based B-band observations to investigate how the color dispersion
relates to global galaxy properties. The intenal color dispersion generally
correlates with transformations in galaxy morphology as a function of
wavelength, i.e., it quantifies the morphological K-correction. Mid-type spiral
galaxies exhibit the highest dispersion in their internal colors, which stems
from differences in the bulge, disk, and spiral-arm components. Irregulars and
late-type spirals show moderate internal color dispersion, which implies that
young stars generally dominate the colors. Ellipticals, lenticulars, and
early-type spirals generally have low or negligible internal color dispersion,
which indicates that the stars contributing to the UV-to-optical emission have
a very homogeneous distribution. We discuss the application of the internal
color dispersion to high-redshift galaxies in deep, Hubble Space Telescope
images. By simulating local galaxies at cosmological distances, many of the
galaxies have luminosities that are sufficiently bright at rest--frame optical
wavelengths to be detected within the limits of the currently deepest
near-infrared surveys even with no evolution. Under assumptions that the
luminosity and color evolution of the local galaxies conform with the measured
values of high-redshift objects, we show that galaxies' intrinsic internal
color dispersion remains measurable out to z ~ 3.Comment: Accepted for publication in the Astrophysical Journal. 41 pages, 13
figures (3 color). Full resolution version (~8 Mb) available at
http://mips.as.arizona.edu/~papovich/papovich_astroph.p
Survey of Canada Goose Feces for Presence of \u3cem\u3eGiardia\u3c/em\u3e
As resident Canada goose (Branta canadensis) populations increase throughout North America, so do the health and environmental risks associated with goose feces. Previous studies suggest that goose feces may be a conduit for transmitting Giardia, a protozoan that is parasitic to humans. We surveyed fecal droppings from free-ranging resident Canada geese for Giardia spp. at 9 sites in the Triangle area (Raleigh, Durham, and Chapel Hill) of North Carolina in 2007 and 2008. Samples (n = 234) were tested using the ProSpect® Giardia EZ Microplate Assay, and there were no positives. Our results indicate that risk of zoonotic giardiasis from Canada goose feces in the Triangle area of North Carolina is low
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Draft Genome Sequence of Rhodococcus sp. Strain ATCC 49988, a Quinoline-Degrading Bacterium.
We report here the 4.9-Mb genome sequence of a quinoline-degrading bacterium, Rhodococcus sp. strain ATCC 49988. The draft genome data will enable the identification of genes and future genetic modification to enhance traits relevant to heteroaromatic compound degradation
Automated reconstruction and comparison of metabolic models for diverse fungal genomes
info:eu-repo/semantics/publishedVersio
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