405 research outputs found
Aluminum-silicon eutectic alloy improves electrical and mechanical contact to silicon carbide
Alloy contact layer is made at relatively low temperature and has good wetting characteristics. Contacts adhere well to silicon carbide surface, penetrating about 300 to 500 angstroms into it. Contacts are ohmic on p-type silicon carbide and blocking on n-type
Copper-titanium eutectic alloy improves electrical and mechanical contact to silicon carbide
Contact preparation at low temperatures is possible with the use of a copper-titanium eutectic alloy. Contacts formed with this alloy are ohmic on p-type silicon carbide and rectifying on n-type
What is the probability of connecting two points ?
The two-terminal reliability, known as the pair connectedness or connectivity
function in percolation theory, may actually be expressed as a product of
transfer matrices in which the probability of operation of each link and site
is exactly taken into account. When link and site probabilities are and
, it obeys an asymptotic power-law behavior, for which the scaling factor
is the transfer matrix's eigenvalue of largest modulus. The location of the
complex zeros of the two-terminal reliability polynomial exhibits structural
transitions as .Comment: a few critical polynomials are at the end of the .tex source fil
Dust and gas in luminous infrared galaxies - results from SCUBA observations
We present new data taken at 850 m with SCUBA at the JCMT for a sample
of 19 luminous infrared galaxies. Fourteen galaxies were detected. We have used
these data, together with fluxes at 25, 60 and 100 m from IRAS, to model
the dust emission. We find that the emission from most galaxies can be
described by an optically thin, single temperature dust model with an exponent
of the dust extinction coefficient () of
. A lower is required to model the dust
emission from two of the galaxies, Arp 220 and NGC 4418. We discuss various
possibilities for this difference and conclude that the most likely is a high
dust opacity. In addition, we compare the molecular gas mass derived from the
dust emission, , with the molecular gas mass derived from the CO
emission, , and find that is on average a factor 3 higher than
.Comment: 10 pages, 6 figures, latex, with MN-macros, accepted by MNRAS -
revised version (changed flux values for some galaxies
Near-infrared line imaging of the starburst galaxies NGC 520, NGC 1614 and NGC 7714
We present high spatial resolution (0.6 arcsec) near-infrared broad-band JHK
images and Br_gamma 2.1661 micron and H_2 1-0 S(1) 2.122 micron emission line
images of the nuclear regions in the interacting starburst galaxies NGC 520,
NGC 1614 and NGC 7714. The near-infrared emission line and radio morphologies
are in general agreement, although there are differences in details. In NGC
1614, we detect a nuclear double structure in Br_gamma, in agreement with the
radio double structure. We derive average extinctions of A(K) = 0.41 and A(K) =
0.18 toward the nuclear regions of NGC 1614 and NGC 7714, respectively. For NGC
520, the extinction is much higher, A(K) = 1.2 - 1.6. The observed H_2/Br_gamma
ratios indicate that the main excitation mechanism of the molecular gas is
fluorescence by intense UV radiation from clusters of hot young stars, while
shock excitation can be ruled out.
The starburst regions in all galaxies exhibit small Br_gamma equivalent
widths. Assuming a constant star formation model, even with a lowered upper
mass cutoff of M_u = 30 M_o, results in rather old ages (10 - 40 Myr), in
disagreement with the clumpy near-infrared morphologies. We prefer a model of
an instantaneous burst of star formation with M_u = 100 M_o, occurring 6 - 7
Myr ago, in agreement with previous determinations and with the detection of
W-R features in NGC 1614 and NGC 7714. Finally, we note a possible systematic
difference in the amount of hot molecular gas between starburst and Seyfert
galaxies.Comment: 13 pages, A&A, accepte
The Large-Scale Atomic and Molecular Gas in the Circinus Galaxy
We have used the ATCA and the SEST to map the large-scale atomic and
molecular gas in the nearby Circinus galaxy. The HI mosaic of Circinus exhibits
the warps in position angle and inclination revealed in the single-pointing
image, both of which appear to settle beyond the inner 30 kpc which was
previously imaged. The molecular gas has been mapped in both the CO
transitions, where we derive a total molecular gas mass of ~2e9 Mo. Within a
radius of 3 kpc, i.e. where CO was clearly detected, the molecular fraction
climbs steeply from ~0.7 to unity with proximity to the nucleus. Our HI mosaic
gives an atomic gas mass of ~6e9 Mo which is 70% of the fully mapped single
dish value. The total neutral gas mass to dynamical mass ratio is therefore 3%,
consistent with the SAS3 classification of Circinus. The high (molecular) gas
mass fraction found previously, only occurs close to the central ~0.5 kpc and
falls to < 10% within and outwith this region, allaying previous concerns
regarding the validity of applying the Galactic conversion ratio to Circinus.
The rotation curve, as traced by both the HI and CO, exhibits a steep dip at ~1
kpc, the edge of the atomic/molecular ring, within which the star-burst is
occurring. We find the atomic and molecular gases to trace different
kinematical features and believe that the fastest part of the sub-kpc ring
consists overwhelmingly of molecular gas. Beyond the inner kpc, the velocity
climbs to settle into a solid body rotation at >10 kpc. Most of the starlight
emanates from within this radius and so much of the dynamical mass, which
remains climbing to the limit of our data (>50 kpc), must be due to the dark
matter halo.Comment: 13 pages, MNRAS in pres
Određivanje aflatoksina, okratoksina A, fumonizina i zearalenona u žitaricama i krmivu primjenom kompetetivnoga direktnog imunoenzimatskog testa (CD-ELISA) i tankoslojne kromatografije (TLC)
Aspergillus, Penicillium, and Fusarium species frequently contaminate crops. For this reason mycotoxins such as afl atoxins (AFs), ochratoxin A (OTA), fumonisins (FBs), and zearalenone (ZEA) are found in food and feed in a wide range of concentrations, depending on environmental and storage conditions.
Consumption of mycotoxin-contaminated food and feed has been associated with acute and chronic poisoning and carcinoma. The aim of this study was to determine the incidence and co-occurrence of AFs
(B1+B2+G1+G2), OTA, FBs (B1+B2+B3), and ZEA in 37 samples of cereals and feed randomly collected in 2007 from households of an endemic nephropathy (EN) area in Croatia. The mycotoxins were determined using the competitive direct ELISA test (CD-ELISA) in combination with thin-layer chromatography (TLC). The most frequent mycotoxin was ZEA (92 %, mean 318.3 μg kg-1), followed by FBs (27 %, 3690 μg kg-1), AFs (24.3 %, 4.6 μg kg-1), and OTA (16.2 %, 9.8 μg kg-1). Levels of AFs, ZEA, and FBs detected by CD-ELISA signifi cantly correlated with the TLC results. However, only one OTA-positive sample was confi rmed by TLC due to its high limit of detection. The levels of these mycotoxins were below the permissible limit for animal feed. Twenty-nine percent of cereals were contaminated with FBs, OTA, or ZEA in mass fractions above the permissible limit for humans. Co-occurrence of two toxins
varied between 4.2 % and 54 % and of three between 4.2 % and 7.6 %. Prolonged co-exposure to AFs, OTA, FBs, and ZEA might increase the risk of various chronic diseases.Vrste plijesni iz rodova Aspergillus, Penicillium i Fusarium česti su kontaminanti usjeva te na takvim supstratima tvore mikotoksine. Stoga su žitarice i krmiva često kontaminirana afl atoksinima (AFs),
okratoksinom A (OTA), fumonizinima (FBs) i zearalenonom (ZEA) u različitim koncentracijama ovisno o mikroklimatskim uvjetima na polju i u skladištu. Konzumiranje hrane kontaminirane mikotoksinima
često je povezano s akutnim ili kroničnim trovanjima, ali i s razvojem karcinoma. Cilj ovog rada bio je odrediti istodobnu pojavnost AFs (B1+B2+G1+G2), OTA, FBs (B1+B2+B3) i ZEA u uzorcima žitarica i krme (N=37) koji su nasumično skupljeni u individualnim domaćinstvima na području endemske nefropatije (EN) u Hrvatskoj (2007). Za određivanje navedenih mikotoksina korišten je kompetitivni direktni ELISA-test (CD-ELISA) u kombinaciji s tankoslojnom kromatografi jom (TLC). Najzastupljeniji mikotoksin bio
je ZEA (92 %, srednja koncentracija 318.3 μg kg-1), nakon čega slijede FBs (27 %, 3690 μg kg-1), AFs (24.3 %, 4.6 μg kg-1) te OTA (16.2 %, 9.8 μg kg-1). Koncentracije AFs, FBs i ZEA određene CD-ELISA-testom statistički značajno koreliraju s rezultatima dobivenim s TLC. OTA je potvrđen metodom TLC samo u jednom uzorku zbog visokog limita detekcije. Dokazane koncentracije su ispod razina dopuštenih za krmiva, dok je 29 % uzoraka žitarica sadržavalo FBs, OTA ili ZEA u koncentracijama iznad dopuštenih u hrani za ljude. Kokontaminacija s dvama odnosno trima toksinima varirala je između 4.2 % i 54 % odnosno između 4.2 % i 7.6 %. Dugotrajni unos AFs, OTA, FBs i ZEA putem hrane može povećati rizik od razvoja različitih kroničnih bolesti zbog njihova mogućega sinergističkog djelovanja
A Chromosome-Length Reference Genome for the Endangered Pacific Pocket Mouse Reveals Recent Inbreeding in a Historically Large Population
High-quality reference genomes are fundamental tools for understanding population history, and can provide estimates of genetic and demographic parameters relevant to the conservation of biodiversity. The federally endangered Pacific pocket mouse (PPM), which persists in three small, isolated populations in southern California, is a promising model for studying how demographic history shapes genetic diversity, and how diversity in turn may influence extinction risk. To facilitate these studies in PPM, we combined PacBio HiFi long reads with Omni-C and Hi-C data to generate a de novo genome assembly, and annotated the genome using RNAseq. The assembly comprised 28 chromosome-length scaffolds (N50 = 72.6 MB) and the complete mitochondrial genome, and included a long heterochromatic region on chromosome 18 not represented in the previously available short-read assembly. Heterozygosity was highly variable across the genome of the reference individual, with 18% of windows falling in runs of homozygosity (ROH) >1 MB, and nearly 9% in tracts spanning >5 MB. Yet outside of ROH, heterozygosity was relatively high (0.0027), and historical Ne estimates were large. These patterns of genetic variation suggest recent inbreeding in a formerly large population. Currently the most contiguous assembly for a heteromyid rodent, this reference genome provides insight into the past and recent demographic history of the population, and will be a critical tool for management and future studies of outbreeding depression, inbreeding depression, and genetic load
Utilisation of an operative difficulty grading scale for laparoscopic cholecystectomy
Background
A reliable system for grading operative difficulty of laparoscopic cholecystectomy would standardise description of findings and reporting of outcomes. The aim of this study was to validate a difficulty grading system (Nassar scale), testing its applicability and consistency in two large prospective datasets.
Methods
Patient and disease-related variables and 30-day outcomes were identified in two prospective cholecystectomy databases: the multi-centre prospective cohort of 8820 patients from the recent CholeS Study and the single-surgeon series containing 4089 patients. Operative data and patient outcomes were correlated with Nassar operative difficultly scale, using Kendall’s tau for dichotomous variables, or Jonckheere–Terpstra tests for continuous variables. A ROC curve analysis was performed, to quantify the predictive accuracy of the scale for each outcome, with continuous outcomes dichotomised, prior to analysis.
Results
A higher operative difficulty grade was consistently associated with worse outcomes for the patients in both the reference and CholeS cohorts. The median length of stay increased from 0 to 4 days, and the 30-day complication rate from 7.6 to 24.4% as the difficulty grade increased from 1 to 4/5 (both p < 0.001). In the CholeS cohort, a higher difficulty grade was found to be most strongly associated with conversion to open and 30-day mortality (AUROC = 0.903, 0.822, respectively). On multivariable analysis, the Nassar operative difficultly scale was found to be a significant independent predictor of operative duration, conversion to open surgery, 30-day complications and 30-day reintervention (all p < 0.001).
Conclusion
We have shown that an operative difficulty scale can standardise the description of operative findings by multiple grades of surgeons to facilitate audit, training assessment and research. It provides a tool for reporting operative findings, disease severity and technical difficulty and can be utilised in future research to reliably compare outcomes according to case mix and intra-operative difficulty
PMAS integral field spectroscopy of luminous infrared galaxies. I.- The atlas
In this paper we present PMAS optical (3800-7200A) IFS of the northern
hemisphere portion of a volume-limited sample of 11 LIRGs. The PMAS
observations typically cover the central ~5kpc and are complemented with
HST/NICMOS images. For most LIRGs in our sample, the peaks of the continuum and
gas (e.g., Halpha, [NII]) emissions coincide, unlike what is observed in local,
strongly interacting ULIRGs. The only exceptions are galaxies with
circumnuclear rings of star formation where the most luminous Halpha emitting
regions are found in the rings rather than in the nuclei, and the displacements
are well understood in terms of differences in the stellar populations. A large
fraction of the nuclei of these LIRGs are classified as LINER and intermediate
LINER/HII, or composite objects. The excitation conditions of the integrated
emission depend on the relative contributions of HII regions and the diffuse
emission to the line emission over the PMAS FoV. Galaxies dominated by high
surface-brightness HII regions show integrated HII-like excitation. A few
galaxies show slightly larger integrated [NII]/Halpha and [SII]/Halpha line
ratios than the nuclear ones, probably because of more contribution from the
diffuse emission. The Halpha velocity fields over the central few kpc are
generally consistent, at least to first order, with rotational motions. The
velocity fields of most LIRGs are similar to those of disk galaxies, in
contrast to the highly perturbed fields of most local, strongly interacting
ULIRGs. The peak of the Halpha velocity dispersion coincides with the position
of the nucleus and is likely to be tracing mass. All these results are similar
to the properties of z~1 LIRGs, and they highlight the importance of detailed
studies of flux-limited samples of local LIRGs. (Abridged)Comment: Accepted for publication in Astronomy and Astrophysic
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