34 research outputs found
Tidally Induced Offset Disks in Magellanic Spiral Galaxies
Magellanic spiral galaxies are a class of one-armed systems that often
exhibit an offset stellar bar, and are rarely found around massive spiral
galaxies. Using a set of N-body and hydrodynamic simulations we consider a
dwarf-dwarf galaxy interaction as the driving mechanism for the formation of
this peculiar class of systems. We investigate here the relation between the
dynamical, stellar and gaseous disk center and the bar. In all our simulations
the bar center always coincides with the dynamical center, while the stellar
disk becomes highly asymmetric during the encounter causing the photometric
center of the Magellanic galaxy disk to become mismatched with both the bar and
the dynamical center. The disk asymmetries persist for almost 2 Gyrs, the time
that it takes for the disk to be re-centered with the bar, and well after the
companion has passed. This explains the nature of the offset bar found in many
Magellanic-type galaxies, including the Large Magellanic Cloud (LMC) and NGC
3906. In particular, these results, once applied to the LMC, suggest that the
dynamical center should reside in the bar center instead of the HI center as
previously assumed, pointing to a variation in the current estimate of the
north component of the LMC proper motion.Comment: 12 pages, 8 figures, corrected for referee comment
Evolution of the Kdo2-lipid A biosynthesis in bacteria
<p>Abstract</p> <p>Background</p> <p>Lipid A is the highly immunoreactive endotoxic center of lipopolysaccharide (LPS). It anchors the LPS into the outer membrane of most Gram-negative bacteria. Lipid A can be recognized by animal cells, triggers defense-related responses, and causes Gram-negative sepsis. The biosynthesis of Kdo<sub>2</sub>-lipid A, the LPS substructure, involves with nine enzymatic steps.</p> <p>Results</p> <p>In order to elucidate the evolutionary pathway of Kdo<sub>2</sub>-lipid A biosynthesis, we examined the distribution of genes encoding the nine enzymes across bacteria. We found that not all Gram-negative bacteria have all nine enzymes. Some Gram-negative bacteria have no genes encoding these enzymes and others have genes only for the first four enzymes (LpxA, LpxC, LpxD, and LpxB). Among the nine enzymes, five appeared to have arisen from three independent gene duplication events. Two of such events happened within the Proteobacteria lineage, followed by functional specialization of the duplicated genes and pathway optimization in these bacteria.</p> <p>Conclusions</p> <p>The nine-enzyme pathway, which was established based on the studies mainly in <it>Escherichia coli </it>K12, appears to be the most derived and optimized form. It is found only in <it>E. coli </it>and related Proteobacteria. Simpler and probably less efficient pathways are found in other bacterial groups, with Kdo<sub>2</sub>-lipid A variants as the likely end products. The Kdo<sub>2</sub>-lipid A biosynthetic pathway exemplifies extremely plastic evolution of bacterial genomes, especially those of Proteobacteria, and how these mainly pathogenic bacteria have adapted to their environment.</p
Ontology-based Navigation of Bibliographic Metadata
This paper describes the work done within the Food and
Agriculture Organization of the United Nations (FAO) on providing an
ontology-based navigation for the Food, Nutrition and Agriculture
(FNA) Journal. The aim of the revised navigation was to provide more
efficient and effective browsing of the Food and Nutrition Publications
using a knowledge model to guide the user with concepts and
relationships relevant to a specific subject area. With this approach, data
from two different bibliographical databases was merged, unified and
presented to the user with improved services. A preliminary metadata
merge was needed to combine all the information into one system in
order to produce a metadata-ontology. Resource Description
Framework Schema (RDFS) was chosen to exploit semantic
relationships, e.g. the possibilities of browsing the data in different
ways (by keywords, categories, authors, etc.), and the creation of a
multilingual concept-based advanced search
The Lyman Alpha Reference Sample. VIII. Characterizing Lyman-Alpha Scattering in Nearby Galaxies
We examine the dust geometry and Ly{\alpha} scattering in the galaxies of the
Lyman Alpha Reference Sample (LARS), a set of 14 nearby (0.02 < < 0.2)
Ly{\alpha} emitting and starbursting systems with Hubble Space Telescope
Ly{\alpha}, H{\alpha}, and H{\beta} imaging. We find that the global dust
properties determined by line ratios are consistent with other studies, with
some of the LARS galaxies exhibiting clumpy dust media while others of them
show significantly lower Ly{\alpha} emission compared to their Balmer
decrement. With the LARS imaging, we present Ly{\alpha}/H{\alpha} and
H{\alpha}/H{\beta} maps with spatial resolutions as low as 40 pc, and
use these data to show that in most galaxies, the dust geometry is best modeled
by three distinct regions: a central core where dust acts as a screen, an
annulus where dust is distributed in clumps, and an outer envelope where
Ly{\alpha} photons only scatter. We show that the dust that affects the escape
of Ly{\alpha} is more restricted to the galaxies' central regions, while the
larger Ly{\alpha} halos are generated by scattering at large radii. We present
an empirical modeling technique to quantify how much Ly{\alpha} scatters in the
halo, and find that this "characteristic" scattering distance correlates with
the measured size of the Ly{\alpha} halo. We note that there exists a slight
anti-correlation between the scattering distance of Ly{\alpha} and global dust
properties.Comment: 32 pages, 51 figures, accepted to Ap
The Lyman Alpha Reference Sample: III. Properties of the Neutral ISM from GBT and VLA Observations
We present new H I imaging and spectroscopy of the 14 UV-selected
star-forming galaxies in the Lyman Alpha Reference Sample (LARS), aimed for a
detailed study of the processes governing the production, propagation, and
escape of Ly photons. New H I spectroscopy, obtained with the 100m
Green Bank Telescope (GBT), robustly detects the H I spectral line in 11 of the
14 observed LARS galaxies (although the profiles of two of the galaxies are
likely confused by other sources within the GBT beam); the three highest
redshift galaxies are not detected at our current sensitivity limits. The GBT
profiles are used to derive fundamental H I line properties of the LARS
galaxies. We also present new pilot H I spectral line imaging of 5 of the LARS
galaxies obtained with the Karl G. Jansky Very Large Array (VLA). This imaging
localizes the H I gas and provides a measurement of the total H I mass in each
galaxy. In one system, LARS 03 (UGC 8335 or Arp 238), VLA observations reveal
an enormous tidal structure that extends over 160 kpc from the main interacting
systems and that contains 10 M of H I. We compare various H I
properties with global Ly quantities derived from HST measurements. The
measurements of the Ly escape fraction are coupled with the new direct
measurements of H I mass and significantly disturbed H I velocities. Our
robustly detected sample reveals that both total H I mass and linewidth are
tentatively correlated with key Ly tracers. Further, on global scales,
these data support a complex coupling between Ly propagation and the H
I properties of the surrounding medium.Comment: Preprint form, 16 figures, accepted in Ap
The Lyman alpha reference sample. VII. Spatially resolved H kinematics
We present integral field spectroscopic observations with the Potsdam Multi
Aperture Spectrophotometer of all 14 galaxies in the Lyman Alpha
Reference Sample (LARS). We produce 2D line of sight velocity maps and velocity
dispersion maps from the Balmer (H) emission in our data
cubes. These maps trace the spectral and spatial properties of the LARS
galaxies' intrinsic Ly radiation field. We show our kinematic maps
spatially registered onto the Hubble Space Telescope H and Lyman
(Ly) images. Only for individual galaxies a causal connection
between spatially resolved H kinematics and Ly photometry can
be conjectured. However, no general trend can be established for the whole
sample. Furthermore, we compute non-parametric global kinematical statistics --
intrinsic velocity dispersion , shearing velocity ,
and the ratio -- from our kinematic maps. In
general LARS galaxies are characterised by high intrinsic velocity dispersions
(54\,km\,s median) and low shearing velocities (65\,km\,s
median). values range from 0.5 to 3.2 with an
average of 1.5. Noteworthy, five galaxies of the sample are dispersion
dominated systems with and are thus
kinematically similar to turbulent star forming galaxies seen at high redshift.
When linking our kinematical statistics to the global LARS Ly
properties, we find that dispersion dominated systems show higher Ly
equivalent widths and higher Ly escape fractions than systems with
. Our result indicates that turbulence in
actively star-forming systems is causally connected to interstellar medium
conditions that favour an escape of Ly radiation.Comment: 26 pages, 15 figures, accepted for publication in A&
The Neutral Gas Dynamics of the Nearby Magellanic Irregular Galaxy UGCA 105
We present new low-resolution HI spectral line imaging, obtained with the
Karl G. Jansky Very Large Array (JVLA), of the star-forming Magellanic
irregular galaxy UGCA 105. This nearby (D = 3.39+/-0.25 Mpc), low mass
[M_HI=(4.3+/-0.5)x10^8 Solar masses] system harbors a large neutral gas disk
(HI radius ~7.2 kpc at the N_HI=10^20 cm^-2 level) that is roughly twice as
large as the stellar disk at the B-band R_25 isophote. We explore the neutral
gas dynamics of this system, fitting tilted ring models in order to extract a
well-sampled rotation curve. The rotation velocity rises in the inner disk,
flattens at 72+/-3 km/s, and remains flat to the last measured point of the
disk (~7.5 kpc). The dynamical mass of UGCA 105 at this outermost point,
(9+/-2)x10^9 Solar masses, is ~10 times as large as the luminous baryonic
components (neutral atomic gas and stars). The proximity and favorable
inclination (55 degrees) of UGCA 105 make it a promising target for
high-resolution studies of both star formation and rotational dynamics in a
nearby low-mass galaxy.Comment: The Astronomical Journal, in pres